The galaxy presents as a relatively smooth, concentrated object with a generally elliptical morphology. The galaxy exhibits a dominant, centrally concentrated bulge. There is no evidence of strong spiral arm structure, bar features, or significant dust lanes. Color gradients suggest a population of older stars throughout the galaxy, with the core showing more yellow-red color characteristics of older stellar populations. The galaxy has a relatively smooth profile, indicating it is most likely an elliptical galaxy, viewed from the side. There is no major evidence of any merging systems.