Lightcurve analysis gave a well-defined rotation period of 11.680 hours with a brightness variation of 0.22 magnitude (). Observations at the Italian Bassano Bresciano Observatory in December 2011 measured a concurring period 11.674 with an amplitude of 0.30 magnitude ().
Lightcurve analysis, which is used to determine the rotation period and brightness variation of celestial objects, yielded a well-defined rotation period of 11.680 hours with a brightness variation of 0.22 magnitude (). Observations at the Italian Bassano Bresciano Observatory in December 2011 measured a concurring period 11.674 with an amplitude of 0.30 magnitude ().