 In November 2017, a rotational lightcurve of "Lova" was obtained from photometric observations by Tom Polakis at the Command Module Observatory in Arizona.Lightcurve analysis gave a well-defined rotation period of hours with a brightness variation of magnitude ().While not being a slow rotator, which have periods of 100 or more hours, "Lova"s period is significantly longer than the vast majority of asteroids, which rotate within 2.2 to 20 hours once around their axis.