The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. Its overall color profile indicates a population of older stars, with a general lack of blue light associated with recent star formation. There is a slight elongation to its shape. No spiral arm structures or significant dust lanes are discernible within the galaxy's image. The galaxy exhibits a consistent color gradient across its extent, showing a gradual transition from a brighter central region to a fainter outer halo. There is no visual evidence of any ongoing merger activity or major tidal disturbances, although a very minor asymmetry cannot be ruled out. The galaxy exhibits characteristics of a mature, relatively undisturbed system.
