 It gave a rotation period of 10.46 hours with a brightness variation of 0.14 magnitude ().The asteroid was also observed by French amateur astronomer Pierre Antonini in January 2007, and by the Spanish "Observadores de Asteroides" (OBAS) group in February 2016.However, the obtained lightcurves were only fragmentary and gave a divergent period of 23 and 35.2 hours with and amplitude of 0.04 and 0.13 magnitude, respectively ().