The galaxy presents as a largely smooth, elliptical-like structure. It exhibits a concentrated central bulge, which appears yellowish-orange in color, possibly indicative of an older stellar population. The outer regions show a gradual decrease in brightness and a bluer hue, suggesting the presence of some younger stars or ongoing star formation. The galaxy appears relatively undisturbed with no obvious signs of a major merger or tidal interactions. There is a very slight indication of a disk or arm like formation on the far right of the galaxy, however this is very slight. Overall, it displays a general elliptical morphology with some evidence of a more complex formation history.
