The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated, bright central region that gradually fades outwards into a more diffuse halo. The color profile suggests a redder, more evolved stellar population, particularly within the core. There is no apparent spiral structure or significant dust lane obscuration visible. The galaxy appears relatively undisturbed, lacking any significant signs of tidal interactions or mergers. It seems to be a well-defined, isolated system dominated by older stars.
