The galaxy exhibits an elliptical morphology, displaying a smooth, centrally concentrated luminosity profile. The central region appears yellowish, suggesting a population of older stars and a lack of significant ongoing star formation. The outer regions fade gradually into a faint, diffuse halo with a slightly bluish tint. This bluer hue in the periphery hints at a younger stellar population compared to the core, with the galaxy being seen at a distance where fine morphological details are not easily resolved. No distinct spiral arms or prominent dust lanes are visible. The overall appearance suggests a relatively evolved system that has experienced some past disturbance.
