The galaxy presents as a centrally concentrated object with a generally smooth morphology. The core region exhibits a bright, concentrated luminosity. This suggests a high density of stars and possibly an active galactic nucleus, but the resolution is insufficient to confirm.

Moving outward from the core, the galaxy fades in luminosity, forming a diffuse halo. There is minimal evidence of spiral arms or distinct disk-like features. The overall shape appears generally round, possibly slightly elliptical.

The galaxy shows a color gradient, with the core exhibiting a yellower/redder hue, and the outer regions transitioning toward a bluer color. This suggests a possible difference in stellar populations, with older, redder stars concentrated toward the core and younger, bluer stars more dispersed in the halo. However, the image quality is not high enough to confirm any fine details. There is no clear evidence of recent major merger activity, although some minor disturbances cannot be ruled out completely based on the smoothness of the general structure.
