The galaxy appears as an elliptical structure with a smooth, diffuse light distribution. It exhibits a moderate degree of ellipticity, appearing somewhat elongated rather than perfectly circular. The central region displays a brighter concentration of light, indicating a nucleus or a bulge component. The color profile suggests a population of older stars, evidenced by the yellowish-red hue dominant throughout the galaxy. There is little indication of spiral arms or significant dust lanes. Faint, diffuse light extends outwards from the central region, gradually fading into the background. No signs of major mergers or tidal disturbances are apparent in this image.
