The galaxy presents as an elliptical morphology, with a smooth, concentrated light profile. The core is a bright, yellow-white, suggesting an older stellar population. The halo exhibits a gradual decrease in luminosity moving outward from the center, transitioning to a faint, diffuse edge. No distinct spiral arms or dust lanes are apparent. There are potentially minor irregularities or tidal features, but the dominant impression is of a relaxed, relatively undisturbed system. The color index indicates a redder composition compared to typical spiral galaxies, supporting the interpretation of an aging stellar population and relatively low recent star formation activity. The overall symmetry is slightly off-center, with a possible faint extension on the right side of the image. The galaxy is neither extremely flattened nor perfectly spherical, presenting an intermediate ellipticity.
