The galaxy presents as a somewhat elliptical or lenticular structure. The central bulge exhibits a high degree of luminosity, appearing quite bright and concentrated. Moving outwards, there's a gradual decrease in luminosity, with no readily apparent spiral arm structure or distinct features. The overall color profile suggests a population of older stars, likely a result of limited ongoing star formation. There is a subtle, faint halo surrounding the central region, however it's difficult to discern it's composition from this image alone. There is little evidence to suggest any recent or ongoing major mergers or disturbances. The galaxy appears relatively smooth and undisturbed in its overall morphology.
