The galaxy presents an overall elliptical morphology, appearing largely smooth and lacking significant spiral arm structures. The light distribution is centrally concentrated, with a bright, yellowish core suggesting a population of older stars. Fainter, bluish-white light extends outwards from the core in a somewhat elongated shape, indicating the presence of a younger stellar population and potentially some ongoing star formation, albeit at a moderate level. There is a subtle suggestion of a disk-like component to the galaxy, primarily based on the relatively confined extent of the bluer light. No strong tidal features or evidence of recent major mergers are apparent, but there might be very subtle asymmetries that are indicative of a minor interaction. The color gradient suggests that the central region is more dominated by older stars while the outer regions show signs of ongoing star formation.
