 In the taxonomic classification based on near-infrared colors from the MOVIS-catalog, the asteroid is a Cgx-subtype that is closest to a carbonaceous C-type and somewhat similar to a uncommon G-type and X-type asteroid.The MOVIS catalog was created from data gather by the VISTA Hemisphere Survey conducted with the VISTA telescope at Paranal Observatory in Chile.In October 2017, a rotational lightcurve of "Ceraskia" was obtained from photometric observations by Matthieu Conjat at Nice Observatory in France.