The galaxy appears to be a relatively smooth, centrally concentrated system. The light profile suggests an elliptical morphology, with a bright, spheroidal core that gradually fades into the outer regions. There is very little, if any, indication of spiral arm structure or a prominent disk component based on color and morphology. The overall color is somewhat redder, implying a higher population of older stars and a lack of significant ongoing star formation. There are no apparent major tidal features or significant morphological distortions to indicate a recent major merger, though the existence of minor disturbances cannot be ruled out based on image alone. The galaxy appears undisturbed, presenting a regular and symmetrical form. The color gradients across the galaxy seem consistent with typical ellipticals.