The asteroid has been observed in 3 more stellar occultation events.[6]
Photometric observations of this asteroid in 2016 producedlightcurves indicating arotation period of 9.9 hours with anamplitude variation of 0.18 in magnitude. This result matched previous determinations of the spin rate. The lightcurve was found to vary over the observation period as the viewing angle changed, suggesting the shadowing of topographic features.[7]
^Warner, Brian D. (December 2007), "Initial Results of a Dedicated H-G Project",The Minor Planet Bulletin, vol. 34, pp. 113–119,Bibcode:2007MPBu...34..113W.
^Pilcher, Frederick (October 2016), "Three Asteroids with Changing Lightcurves: 124 Alkeste, 465 Alekto, and 569 Misa",The Minor Planet Bulletin,43 (4):296–299,Bibcode:2016MPBu...43..296P.