The galaxy presents a relatively smooth and somewhat rounded appearance, indicative of an elliptical morphology, though a faint disk component cannot be ruled out. There is no obvious spiral arm structure apparent in this image. The galaxy exhibits a centrally concentrated luminosity profile, with a gradual decrease in brightness towards its outer regions. Its color index suggests a population of older stars, as its light appears redder. There is no compelling evidence of any ongoing major merging activity or significant tidal disturbances. However, minor disturbances or interactions may be occurring.
