The galaxy presents as an elliptical morphology, dominated by a smooth, centrally concentrated bulge. A slight elongation is apparent, suggesting a deviation from perfect sphericity, potentially an intermediate form between round and cigar-shaped. The light profile displays a radial gradient, with the central region exhibiting a high surface brightness that fades outwards into a more diffuse halo. Color gradients are present, with a redder core transitioning to slightly bluer hues in the outer regions, suggesting some ongoing, albeit limited, star formation activity on the outskirts. There is no obvious evidence of significant tidal features or morphological disturbances indicative of recent major mergers, though the subtle asymmetry might suggest a minor interaction in the past. Overall, the galaxy appears as a relatively quiescent system.
