The galaxy presents as a smooth, centrally concentrated object with an elliptical morphology. The light profile appears to be dominated by an evolved stellar population, inferred from the yellowish-red color, indicative of older stars. There is a slight extension visible along one axis, suggesting a deviation from perfect circularity, but overall, the galaxy exhibits minimal discernible features such as spiral arms or dust lanes. Any signs of recent or ongoing star formation are faint if present at all. There is very little visual evidence of any major tidal interactions or merger events. A slight asymmetry may indicate a possible minor disturbance.
