The galaxy presents as an elliptical morphology, appearing relatively smooth with no discernible spiral arm structures or distinct features. It exhibits a centrally concentrated brightness profile, with luminosity decreasing radially outwards. The galaxy displays a color gradient, appearing more yellow-red towards the center, suggesting a population of older stars. The outer regions are slightly bluer, hinting at the presence of a younger stellar population or some ongoing, albeit low, star formation activity. No significant dust lanes or tidal disturbances are observed, indicating a dynamically relaxed system. The apparent shape is slightly elongated rather than perfectly spherical. Overall, the galaxy appears to be a mature, relatively massive system.
