The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a flattened, elliptical morphology, with a bright nucleus that fades into a diffuse halo. The overall color is moderately red, suggesting an older stellar population. There are no obvious signs of strong spiral arm structure or prominent dust lanes. Subtle disturbances are visible, which may indicate a minor interaction or past merger event. The galaxy appears to be intermediate in roundness, with a slight elongation.
