The galaxy appears to be a relatively smooth, elliptical-type galaxy with a concentrated central bulge. The light distribution is somewhat asymmetrical, with a slight elongation observed. Color gradients suggest a redder central region, indicating a population of older stars or significant dust obscuration. Fainter, bluer features extend away from the bulge and may indicate some current or recent star formation. There may be some minor distortions visible which suggests some ongoing gravitational interaction with a smaller companion. Overall, the galaxy exhibits characteristics of a passively evolving system with evidence for a recent or possible minor merger.
