Efforts to determine the rotation period for this asteroid have produced wildly different results, in large part because the actual period is close to half of an Earth day. A study performed during 2013 showed that thelight curve changed significantly during the observation period, adding to the difficulty. This study gave a synodicrotation period of 14.905 ± 0.001 h.[3]
^Hawkins, Scot; Ditteon, Richard (January 2014), "Asteroid Lightcurve Analysis at the Oakley Observatory - May 2007",Minor Planet Bulletin,41 (1):47–49,Bibcode:2014MPBu...41...47P.