The galaxy presents a generally smooth, elliptical morphology. The core region exhibits a bright, concentrated luminosity profile, transitioning outwards into a less intense, diffuse halo. There is a subtle color gradient visible, with the core appearing more yellow/white, suggestive of an older stellar population, while the outer regions show hints of bluer tones, possibly indicating regions of more recent, albeit modest, star formation activity. The object appears well-rounded in shape, lacking any significant distortions or prominent tidal features that would be indicative of major interactions or ongoing mergers. Overall, the galaxy appears to be a relatively undisturbed, evolved system with minimal ongoing star formation.
