The galaxy presents a largely smooth, elliptical morphology. It appears relatively compact, with a bright, concentrated core region that emits strongly across the visible spectrum. The galaxy exhibits a color gradient, with the central regions displaying a yellowish hue, suggestive of an older stellar population. The outer regions appear slightly bluer, which could be due to the presence of younger stars, or could be attributed to an artifact in the image. There is no evidence of strong spiral arm structure or a prominent disk. Faint, diffuse light extends outwards from the core, fading gradually into the background sky. There is a subtle asymmetry, with the light distribution slightly elongated along one axis. No obvious signs of a recent major merger event are apparent, nor are there distinct tidal tails visible. The object appears to be a single, relatively undisturbed elliptical galaxy.
