Photometric observations of this asteroid at the Palmer Divide Observatory inColorado Springs, Colorado, during 2007 gave alight curve with a period of 6.551 ± 0.002 hours and a brightness variation of 0.05 inmagnitude. This differs somewhat from a 2004 study that gave a period of 6.354 hours, but this difference may be explained by the small magnitude variation which tends to increase the randomizing effect of noise in the data.[6]
^Warner, Brian D. (June 2008), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory - June - October 2007",The Minor Planet Bulletin, vol. 35, no. 2, pp. 56–60,Bibcode:2008MPBu...35...56W.