This asteroid spans a girth of approximately 54 km.[2] It is classified as aK-type asteroid and is aBarbarian, which means it belongs to a class of asteroids of which 234 Barbara is the prototype.[3] Analysis of the asteroidlight curve, based onphotometric data collected during 2009, show arotation period of10.664±0.001 h with a brightness variation of0.30±0.01 inmagnitude.[4]
^Warner, Brian D. (July 2009), "Asteroid Lightcurve Analysis at the Palmer Divide Observatory: 2008 December - 2009 March",Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers,36 (3):109–116,Bibcode:2009MPBu...36..109W.