The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a generally elliptical morphology, trending toward a rounded shape. There is no clear evidence of spiral arm structure or strong disk features. A bright central bulge or core region is apparent, decreasing gradually in luminosity outwards. No significant tidal features or signs of ongoing major merger activity are observed, although a slight asymmetry or minor disturbance might be present in the outer regions. The overall color profile suggests a relatively evolved stellar population, possibly indicating ongoing but subdued star formation.
