The galaxy exhibits a primarily smooth morphology, with a highly concentrated central bulge. The galaxy appears to be elliptical or lenticular in shape, displaying a general lack of distinct spiral arm structure. The core region shows a brighter, reddish hue, which could indicate an older stellar population dominating this area, along with significant dust obscuration. The outer regions of the galaxy fade gradually into the background, showing some faint, diffuse blue light that might hint at a small amount of ongoing star formation in the outer disk. There are no obvious signs of significant tidal disturbances or major mergers, although very subtle minor disturbances cannot be ruled out based on this image alone. The galaxy appears to be relatively isolated in its environment.
