The galaxy presents as a somewhat elliptical, centrally concentrated object. It exhibits a smooth, diffuse appearance with a gradual decline in brightness from the core outwards. There is a lack of discernible spiral arm structure or prominent dust lanes. The color profile suggests a population of older stars, indicated by its yellowish hue. There are some faint, indistinct features that could potentially be a very subtle disk-like structure or minor disturbances. The overall morphology appears relatively undisturbed, without evidence of a major merger or significant tidal interactions. There is a slight elongation along one axis, but the galaxy is mostly round.
