 Lightcurve analysis gave a rotation period of hours with a high brightness variation of magnitude, indicative of an elongated shape ().An alternative period determination of hours with an even higher amplitude of was made by Laurent Bernasconi one month later in October 2010 ().A modeled lightcurve using photometric data from the "Lowell Photometric Database" gave a sidereal period of and two spin axes at (13.0°, −64.0°) and (207.0°, −60.0°) in ecliptic coordinates (λ, β).