The galaxy presents as a somewhat smooth, centrally concentrated object. It displays a generally elliptical morphology, appearing mostly round in shape. There's a slight indication of a color gradient, with a bluer central region that may signify ongoing star formation, and a tendency towards redder hues in the outer regions, potentially indicative of older stellar populations. There is little evidence of spiral arm structure or significant dust lanes. No major disturbances or merger activity is apparent in the image. The galaxy exhibits a relatively compact size for its estimated luminosity, suggesting it is a fairly dense system.
