The galaxy presents as a concentrated central bulge that gradually fades into a less dense outer halo. The overall shape appears to be elliptical, with a fairly smooth texture indicating either an elliptical galaxy or a spiral galaxy viewed face-on with minimal dust obscuration. No spiral arm structures or significant dust lanes are discernible within the image's resolution. The central region exhibits a bright, concentrated luminosity suggesting a high density of stars or potentially an active galactic nucleus. There may be some variation in color from the center of the galaxy to the outer regions, where it appears somewhat redder, but not in the way we might expect to see a blue shift. Overall, it appears to be a fairly mature system, exhibiting characteristics consistent with an early-type galaxy.
