The galaxy presents as a largely elliptical, smooth structure. The primary body exhibits a concentrated central bulge with a diffuse halo. The color profile appears generally redder, suggestive of an older stellar population and reduced star formation activity. There is a slight asymmetry, potentially indicating a minor interaction or disturbance. There is no strong evidence of spiral arm structure or significant dust lanes. Based on its apparent morphology, it is likely a massive galaxy. 
