The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears bright and somewhat reddish in color, potentially indicating an older stellar population. The surrounding galactic halo is more diffuse and appears bluer, which may be indicative of a younger stellar population or ongoing star formation. Overall, the galaxy shows no prominent spiral arm structure or significant dust lanes. There may be a very faint disc structure surrounding the bulge, but is difficult to tell definitively from this image. There are no obvious signs of major recent merger activity, however the overall shape is not perfectly symmetrical and appears disturbed.
