The galaxy presents as a luminous, centrally concentrated system with a smooth overall morphology. Its color profile suggests a relatively evolved stellar population, appearing yellow-white. The light distribution is approximately elliptical, showing a high degree of central concentration with a gradual decrease in brightness outwards. There is little evidence of spiral arm structure, star forming regions, or significant dust lanes. No strong tidal features or signs of recent major merger activity are immediately apparent, although there may be very minor disturbances present. The galaxy exhibits a high degree of roundness.
