The galaxy presents as a relatively smooth, centralized object. Its morphology appears largely spheroidal, with no immediately discernible spiral arms or bar structure. There's a gradual fading of light intensity from the core outwards, suggesting a centrally concentrated stellar distribution. The color profile indicates a predominantly older stellar population, with a yellowish hue dominant in the central regions. The outer edges exhibit a bluer tinge, potentially indicative of some younger stars or ongoing star formation, albeit at a low rate. No signs of major mergers or significant tidal disturbances are readily apparent in the image. The general shape is somewhat elliptical but tending towards round.
