The galaxy presents as a single, somewhat centrally concentrated object with a relatively smooth morphology. The central region exhibits a yellowish-white hue, potentially indicative of an older stellar population. The outer regions display a more diffuse distribution of light with hints of bluer color, which could indicate younger stars are present. Overall, the galaxy appears elliptical or lenticular based on its smooth, rounded shape and lack of discernible spiral arm structure. There are no obvious signs of a major ongoing merger or significant tidal disturbances. Faint color variations may indicate a low level of recent star formation. The overall impression is of a fairly evolved system.
