The galaxy presents as an elliptical or lenticular type, displaying a flattened, disk-like morphology with no prominent spiral arm structure evident. The central region exhibits a bright, concentrated bulge, indicating a relatively high stellar density. This central region appears yellowish, suggesting an older stellar population dominating the core. Moving outwards from the center, the galaxy fades into a more diffuse halo. The outer regions exhibit a bluer hue. The overall shape is elongated with a clear major and minor axis. The galaxy appears relatively smooth in texture, lacking significant dust lanes or distinct star-forming regions. There is a slight asymmetry on either side of the center region that may be indicative of a minor disturbance of some sort.
