The galaxy presents as a largely smooth, elliptical morphology. It exhibits a concentrated, bright core that fades into a more diffuse halo. The color gradient suggests an aging stellar population, with the core exhibiting a yellow hue. There is little to no evidence of spiral arm structure, dust lanes, or significant ongoing star formation within the visible spectrum. The galaxy appears relatively isolated with no obvious signs of tidal interactions or ongoing mergers. It appears as a regular elliptical galaxy based on its round shape, and lack of visible disturbances.
