The rotation period of this asteroid has proven to be a challenge to determine, most likely because it has a complex shape and a rotation axis with a low inclination. However, during the 2015 apparition, photometric measurements of the asteroid were taken from close to the equatorial perspective. The resulting light curve displayed a rotation period of 7.0259±0.0003 h.[2]
^Marciniak, Anna; et al. (June 2016). Różańska, Agata; Bejger, M. (eds.). "Difficult cases in photometric studies of asteroids". 37th Meeting of the Polish Astronomical Society, held 7–10 September 2015 at Adam Mickiewicz University in Poznań, Poland. Proceedings of the Polish Astronomical Society. 3: 84–87. Bibcode:2016pas..conf...84M.