The galaxy presents an elliptical morphology, displaying a smooth, relatively featureless appearance. Its light profile appears centrally concentrated, with a gradual decrease in luminosity towards the outer regions. There is little evidence of spiral arm structures or significant dust lanes. The galaxy exhibits a slightly elongated shape, appearing more oblate than perfectly spherical. The color is predominantly yellow-white, suggestive of an older stellar population, though a hint of bluer light might indicate some ongoing, albeit low-level, star formation. No signs of major mergers or significant tidal disturbances are immediately apparent, though the possibility of minor interactions cannot be ruled out based on this image alone.
