The galaxy presents as an elliptical or lenticular system with a notable bulge and a fainter, extended halo. The core region is bright, with a smooth, concentrated appearance, suggestive of an older stellar population. There is evidence of an elongated structure with a disk-like component, with the galaxy inclined relative to the observer. Some faint spiral arm hints can be seen along the edges of the disk. There are areas of less uniform color distributed throughout the galaxy, possible evidence of minor mergers. Overall, the galaxy appears to be a relatively evolved system, with a substantial amount of older stars.
