The galaxy presents a predominantly smooth, elliptical morphology with a high degree of central concentration. It displays a diffuse, yellowish central region that likely represents an older stellar population. Fainter, bluer light is present, especially along what appears to be an edge. This may indicate some ongoing, albeit limited, star formation. The galaxy shows an intermediate axis ratio, appearing neither perfectly spherical nor highly elongated. There is a slight hint of tidal features, possibly indicating minor gravitational interactions or disturbances. Overall, the galaxy presents a relatively undisturbed form, consistent with a mature system that has largely settled into a stable configuration.
