 The rotation period of this minor planet was first measured by Scott Sheppard in 2003.Light curves obtained by Sheppard at the University of Hawai'i's 2.2-meter telescope gave an ambiguous rotation period of either 6.71 or 13.42 hours, with a brightness variation of 0.14 magnitudes ().The shorter rotation period refers to the single-peaked solution, expected if the brightness variations resulted from albedo spots.