The galaxy presents as a roughly elliptical form, elongated along its major axis. Its core exhibits a bright, concentrated luminosity, characterized by a yellowish-orange hue indicative of an older stellar population. The outer regions of the galaxy appear fainter and bluer, suggesting the presence of a younger stellar population and/or ongoing star formation, although at a relatively low rate. There is no visually apparent indication of strong tidal disturbances or ongoing major mergers, suggesting the galaxy is relatively isolated and undisturbed. It displays a smooth texture, lacking prominent spiral arms or irregular structures. Overall, the galaxy appears as a fairly massive system with a mixed stellar population, dominated by older stars, in a settled state.
