The galaxy appears as a single, moderately compact object with an elliptical morphology. The light is relatively smooth, with a distinct color gradient across its surface. The core region displays a yellowish hue, which may indicate a population of older stars. The outer regions appear slightly redder, suggesting either a metal-rich population of stars or the presence of dust. There is no visual evidence of spiral arms, a bar, or any significant tidal disturbances. The overall appearance suggests a relatively evolved galaxy without ongoing major mergers or significant star formation at the current observation depth and resolution.
