Light curves generated from photometric data indicate a sidereal rotation period of 11.794162±0.000023 h. Preliminary shape models of the asteroid suggest there's a flat region at the southern pole, perhaps indicating a concave area or an impact crater.[4]
References
^Noah Webster (1884) A Practical Dictionary of the English Language
^Warner, Brian D. (October 2008). "A Preliminary Shape and Spin Axis Model for 595 Polyxena". Bulletin of the Minor Planets Section of the Association of Lunar and Planetary Observers. 35 (4): 171–172. Bibcode:2008MPBu...35..171W.