The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, with a bright, somewhat diffuse core. The overall color appears subtly red-shifted, indicative of an older stellar population and potentially lower levels of ongoing star formation. There is a slight elongation in its shape, deviating marginally from a perfect circle, but the galaxy is generally round. No significant spiral arm structure or prominent dust lanes are discernible. There are no signs of major interactions or recent mergers, although very slight disturbances can not be ruled out with this data. Overall, the galaxy appears to be a relatively quiescent system with a considerable mass.
