Photometric observations at the Palmer Divide Observatory
during 2005 showed a best fit rotation period of 79.18 ± 0.02 hours with a brightness
variation of 0.2 ± 0.02 in magnitude. However, some uncertainty remains concerning the reliability of this result.[5]
^Warner, Brian D. (December 2005), "Asteroid lightcurve analysis at the Palmer Divide Observatory - spring 2005", The Minor Planet Bulletin, 32 (4): 90–92, Bibcode:2005MPBu...32...90W.