 Lance Benner suspects it the be a contact binary, composed of two merged objects forming a single asteroid with a lobed shape.Photometric observations by astronomers with the "Mission Accessible Near-Earth Objects Survey" (MANOS) and subsequent evaluation by Brian Warners "Collaborative Asteroid Lightcurve Link", determined that has a rotation period of at least 16 hours.While the object's spectral type is unknown, Warner assumes it to be an S-type asteroid, based on its high albedo, which is typical for stony asteroids.