The galaxy presents a predominantly smooth morphology, with a concentrated central bulge that appears yellowish in color. The light suggests a stellar population dominated by older stars. The galaxy lacks any apparent spiral arm structure or prominent dust lanes. The shape seems to be intermediate between elliptical and disk galaxies. The smooth appearance indicates a lack of ongoing major merging activity. Some minor disturbance cannot be ruled out, though. The relatively round shape indicates a higher probability that it is an elliptical rather than a flattened spiral.