The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. A discernible bulge is present, dominating the overall light profile. The color gradient suggests a relatively old stellar population, with a yellow-red hue dominating the core region. Fainter, diffuse light extends outwards from the central bulge. The lack of distinct spiral arms or prominent dust lanes supports the classification as an early-type galaxy. There are no apparent signs of significant tidal interactions or major disturbances in the galaxy's structure, although a subtle asymmetry in the outer regions may suggest a past minor interaction. The overall structure appears relatively relaxed and evolved.
