The galaxy appears as a roughly elliptical object with a smooth, concentrated light profile. The core region exhibits a yellowish hue, potentially indicative of an older stellar population. The outer regions display a bluer tint, although not pronounced, which could suggest some ongoing, low-level star formation. There's no discernible spiral structure or dust lanes visible. The overall morphology suggests a galaxy that is either an elliptical or a lenticular type, with the smoothness indicating a possible lack of recent major mergers. There is no significant tidal distortion or interaction with any other galaxies. The galaxy is fairly compact, given its considerable luminosity.
