 Lightcurve analysis gave a well-defined rotation period of hours with a brightness variation of magnitude ().Two modeled lightcurves using photometric data from the "Lowell Photometric Database" and from the BlueEye600 robotic telescope at Ondřejov Observatory gave a sidereal period of and , respectively.The modelling of the former gave two poles at (59.0°, −59.0°) and (249.0°, −72.0°), while the one of the latter gave only one pole at (72.0°, −54.0°) in ecliptic coordinates (λ, β).