Based upon the spectra of this object, it is classified as aM-type asteroid, indicating it may be metallic in composition.[5] It may be the remnant of the core of a larger, differentiated asteroid. Near infrared absorption features indicate the presence of variable amounts of low-iron, low-calciumorthopyroxenes on the surface. Trace amounts of water is detected with amass fraction of about 0.13–0.15 wt%.[6] It has an estimated size of around 88 km.[5] With a rotation period of 3.74 hours, it is the fastest rotating asteroid larger than 50 km in diameter.[2]
^abcdefPravec, P.; et al. (May 2012), "Absolute Magnitudes of Asteroids and a Revision of Asteroid Albedo Estimates from WISE Thermal Observations",Asteroids, Comets, Meteors 2012, Proceedings of the conference held May 16–20, 2012 in Niigata, Japan, no. 1667,Bibcode:2012LPICo1667.6089P. See Table 4.
^Hardersen, Paul S.; Gaffey, Michael J.; Abell, Paul A. (January 1983), "Near-IR spectral evidence for the presence of iron-poor orthopyroxenes on the surfaces of six M-type asteroids",Icarus, vol. 175, no. 1, pp. 141–158,Bibcode:2005Icar..175..141H,doi:10.1016/j.icarus.2004.10.017.