Camilla has a very dark surface and primitive carbonaceous composition. A large number of rotational lightcurves of have been obtained from photometric observations since the 1980s. Best rated results gave a short rotation period of 4.844 hours with a brightness amplitude between 0.32 and 0.53 magnitude. Lightcurve analysis indicates that Camilla's pole most likely points towards ecliptic coordinates = with a 10° uncertainty, which gives it an axial tilt of 29°. Follow-up modeling of photometric data gave similar results.
10µ radiometric data collected from Kitt Peak in 1975 gave a first diameter estimate of 209 km. According to the space-based surveys carried out by the Japanese Akari satellite, the Infrared Astronomical SatelliteIRAS and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, as well as observations by the Keck Observatory and photometric modeling, Camilla measures between 185 and 247 kilometers in diameter and its surface has an albedo between 0.160 and 0.294.
On 1 March 2001, a minor-planet moon of Camilla was found by A. Storrs, F. Vilas, R. Landis, E. Wells, C. Woods, B. Zellner, and M. Gaffey using the Hubble Space Telescope. It has been designated but has not yet received an official name. Later observations in September 2005 with the Very Large Telescope allowed the determination of an orbit. Apart from data in infobox, the inclination was found to be 3 ± 1° with respect to an axis pointing towards =. Given the ~10° uncertainty in the actual rotational axis of Camilla, one can say that the orbit's inclination is less than 10°. The satellite is estimated to measure about 11 km in diameter. Assuming a similar density to the primary, this would give it an approximate mass of ~1.5 kg. It has a similar colour to the primary.
Second satellite
In 2016, the discovery of a second satellite of Camilla was reported by astronomers at Cerro Paranal's Very Large Telescope in Chile. It has the provisional designation. Observations were taken between 29 May 2015 and 30 July 2016, using the VLT-SPHERE, the principal instrument attached to the 8-meter "Melipal" unit of the VLT. On 3 out of 5 observation sessions, the new satellite could be detected. The body's orbit has a semi-major axis of 340 kilometers. The "Johnstonsarchive" estimates an orbital period of 12 hours, and derives a diameter for the second satellite of kilometers with a tertiary-to-primary mean-diameter ratio of.
