The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an approximately elliptical morphology, appearing mostly round. The central region displays a yellowish hue, possibly indicative of an older stellar population. Surrounding this core is a diffuse, less luminous halo with a bluish-green tint. The lack of distinct spiral arm structures suggests the galaxy is either an elliptical or lenticular type. There is no obvious evidence of ongoing major mergers or significant tidal disturbances. The overall appearance implies a relatively quiescent system with moderate levels of star formation.
