The galaxy appears to be a relatively smooth, elliptical type. It exhibits a concentrated, bright central bulge that diminishes gradually toward the edges. The light is fairly uniform, lacking distinct spiral arms or prominent dust lanes. The color profile suggests a population of older stars, with a yellow-red hue dominating the central region. The overall structure indicates a mature system where star formation activity is comparatively low. There's no evidence of major mergers or significant tidal disturbances in this image.
