The galaxy presents as a relatively smooth, elliptical morphology. The core exhibits a bright, concentrated luminosity profile, with intensity gradually diminishing outwards. The color appears to be subtly redder or yellower in the central regions, potentially indicating an older stellar population, while the outer regions show some hint of blue that may be the presence of younger stars. The object lacks any obvious spiral arm structures or significant dust lanes. There are no indications of tidal tails or other clear signs of recent major merger events. Small distortions in the symmetry of the isophotes exist, but they are not highly significant, suggesting a minor disturbance. Overall, the galaxy presents a mature and relatively undisturbed appearance.
