The galaxy presents as a roughly elliptical, though not perfectly spherical, structure. A dominant central bulge appears, exhibiting a smooth texture without significant substructure discernible at this resolution. The color profile suggests a population of older stars, leaning towards redder hues, although some bluer regions are present. There are no strong indications of active star formation, though there is some minor star formation activity occurring. Some disturbances are present, indicating possible past minor merger events.
