The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. The central region exhibits a bright, yellowish-white hue, suggesting a substantial population of older stars. The galaxy gradually fades into a less dense, outer halo that extends to approximately twice the radius of the core. This outer region appears slightly bluer in color. There is a slight elongation, but it is mostly round. The galaxy is an isolated object, with no obvious signs of tidal interactions or major morphological disturbances from merging activity. There is a minor asymmetrical structure appearing at the top. Overall, the galaxy appears as a relatively undisturbed elliptical galaxy with a small amount of ongoing star formation in its outer regions.
