The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge that appears yellowish-white, indicating an older stellar population. The outer regions display a gradual decline in surface brightness, with a hint of a disk-like structure or faint arms extending from the central bulge. The color shifts towards a slightly bluer hue in these outer regions, possibly suggesting the presence of younger, hotter stars or ongoing star formation, although at a low rate. There are no significant signs of tidal disturbances or recent merger events.
