The galaxy presents as a centrally concentrated object with a relatively smooth appearance, indicating it may be an elliptical galaxy or a lenticular galaxy seen face-on. The galaxy appears somewhat rounded. There may be some evidence of minor distortions or interactions, given slight asymmetries in the outer regions of the galaxy, but there is no strong sign of a major merger. Based on the observed color profile, there is likely a dominant population of older stars within this galaxy. Star formation is either very low or possibly absent.
