This galaxy appears to be a relatively smooth, elliptical-type galaxy. The central bulge is prominent and exhibits a high surface brightness, appearing nearly circular in projection. There is a gradual decrease in brightness outward from the center. The outer regions of the galaxy show a somewhat elongated shape, with the galaxy appearing to be slightly flattened. The color is generally consistent across the galaxy, trending toward redder hues, indicating an older stellar population. No distinct spiral arms or dust lanes are visible. There are no obvious signs of active star formation. The overall appearance suggests a galaxy that has undergone significant merging in the past.
