The galaxy presents as a centrally concentrated object, displaying a roughly elliptical morphology. A dominant, bright core exhibits a yellowish-orange hue. The light profile appears smooth, with no obvious spiral arm structure. The surrounding halo gradually fades into the background. There appears to be some distortion or asymmetry in the outer halo region, potentially suggesting a minor interaction or disturbance. The overall color gradient implies a relatively old stellar population. There appears to be a subtle dust lane obscuring a portion of the central region.
