The galaxy presents as an elliptical-shaped structure with a smooth, relatively featureless morphology. Color gradients suggest a possible change in stellar populations from the core to the outer regions. The central region appears brighter and exhibits a somewhat yellowish hue. The outer halo exhibits a more extended, bluer color. No spiral arm structures, or significant dust lanes are visible within the observed light. There appears to be no sign of recent major merger activity, although subtle disturbances or tidal features in the outskirts cannot be ruled out definitively given the image resolution. Overall, the galaxy appears to be a relatively massive system, likely composed predominantly of older stellar populations with relatively low current star formation.
