The galaxy presents as a relatively smooth, centrally concentrated system. Its overall shape is elliptical or nearly circular. No distinct spiral arm structures or prominent dust lanes are readily apparent. There is a bright central bulge that dominates the galaxy's luminosity profile, with the light appearing to fade gradually from the core outwards. The galaxy appears to be undergoing low levels of star formation, its color suggests a population dominated by older stars, with some contribution from a younger population. The object displays minimal signs of tidal disturbances or ongoing mergers, indicating it is a relatively relaxed and undisturbed system.
