The galaxy exhibits an elliptical morphology, with a slight elongation along its major axis. The overall color profile suggests a dominant population of older stars, appearing redder in the central bulge region, gradually transitioning to slightly bluer hues in the outer regions, indicative of some ongoing, albeit reduced, star formation. The surface brightness is concentrated towards the center, decreasing steadily outwards. There is a faint disk-like structure, but is not well-defined. No prominent spiral arm structures or strong dust lanes are visible. There is a suggestion of a slight tidal disturbance.
