 Several rotational lightcurves of "Olympiada" have been obtained from photometric observations by American astronomer Brian Warner at his Palmer Divide Observatory in Colorado.Analysis of the best-rated lightcurve from April 2008 gave a rotation period of 3.833 hours with a consolidated brightness variation between 0.27 and 0.66 magnitude (), while the period of his first 1999-observation was later revised from 4.589 to 3.822 hours.For an asteroid of its size, it has a rather fast spin-rate.