The galaxy presents a generally smooth, elliptical morphology. It displays a centrally concentrated luminosity profile, with a bright, yellowish core that gradually fades into the surrounding halo. There is a hint of a flattened disk-like structure. The outer regions exhibit a bluer hue compared to the core, suggesting a population of younger stars and ongoing star formation, albeit at a moderate rate. There is no evidence of strong tidal features, major mergers, or significant disturbances in its shape.
