The galaxy appears as a centrally concentrated, elliptical or lenticular system. It exhibits a smooth, luminous profile with a bright, well-defined core. The light distribution suggests minimal dust lanes or spiral arm structures. The galaxy's color is predominantly yellow-orange, indicative of an older stellar population with a significant proportion of evolved stars. This suggests a relatively low current star formation rate. The object displays a fairly symmetrical structure with only slight deviations from a perfectly rounded shape. There is no obvious evidence of strong tidal interactions or ongoing mergers. The overall morphology points to a system that has largely completed its major phase of star formation, and is likely undergoing a slow process of passive evolution.
