 Lightcurve analysis gave a rotation period of 4.4 hours (twice the original reported period solution of in the R-band) with a brightness amplitude of 0.99 magnitude, which indicates that the body has an elongated, non-spheroidal shape ().The Italian astronomers also determined a V–R color of 0.38.For this asteroid, no observational data has been gathered by the space-based telescopes (IRAS, Akari and WISE) that surveyed large portions of the asteroid belt.