The galaxy presents a generally smooth, elliptical morphology. It is centrally concentrated with a bright, reddish core, possibly indicating an older stellar population in the galactic nucleus. The isophotes surrounding the core are largely regular and rounded, suggesting minimal tidal disruption or recent major merger events. A faint bluish halo extends outwards from the central region, potentially indicative of some ongoing star formation or a younger stellar population in the outer regions of the galaxy. The overall color gradient transitions from red in the center to bluer towards the edges, which could suggest radial variations in stellar population ages and metallicities. There is some subtle asymmetry in the outer halo, but it is not pronounced, and there doesn't seem to be a major interaction event occurring. 
