The galaxy presents as a relatively smooth, centrally concentrated object with an elliptical morphology. The light distribution appears largely homogeneous across the main body, suggesting an older stellar population dominates. There is a bright, concentrated core region, possibly indicating the presence of a supermassive black hole. Evidence of spiral arms or prominent dust lanes is absent. The galaxy is generally round in appearance, showing little elongation. There is a faint, diffuse halo surrounding the bright central region, which likely contains older stars and globular clusters. There does not appear to be any evidence of tidal interactions or ongoing mergers. Overall, this galaxy presents as a well-formed, quiescent system.
