The galaxy presents a primarily smooth morphology, indicating an elliptical or lenticular classification is likely. A slight deviation from perfect sphericity is apparent, leaning more towards an in-between roundness. Weak arm-like features are visible but indistinct. The galaxy exhibits a bright central bulge, with a gradual decrease in luminosity towards the outer regions. The color profile suggests a population of older stars, with a possible ongoing, low level of star formation. No signs of strong tidal interactions or major mergers are immediately apparent.
