The galaxy presents a roughly elliptical morphology, displaying a smooth light distribution that lacks a strong spiral arm structure. It appears to be dominated by a central bulge, characterized by a yellowish-orange hue suggestive of an older stellar population. The overall color index indicates a relatively quiescent galaxy with subdued star formation activity. The galaxy’s light profile suggests a centrally concentrated mass distribution. No prominent tidal features or signs of major recent mergers are evident, though there may be minor disturbances present in the outer regions.
