The galaxy presents as a relatively smooth, rounded structure. Its color appears yellowish-white in the central region, suggesting a significant population of older stars. The galaxy seems to be largely spheroidal, with very little discernible disk structure. Faint disturbances seem to be present, but there are no clearly defined spiral arms or a prominent bar. There is a slight suggestion of tidal features or an ongoing interaction. The presence of these disturbances may indicate minor interactions. Star formation activity appears to be relatively low.