The galaxy appears to be a luminous elliptical, characterized by a smooth, centrally concentrated morphology. The light profile indicates a relatively even distribution, lacking prominent spiral arms or distinct features. The central region displays a yellow-orange hue, possibly indicative of an older stellar population. The galaxy fades gradually towards its outer edges, exhibiting a round shape. There is no visual evidence of ongoing major mergers or significant tidal disturbances; however, subtle asymmetrical features might suggest minor interactions.
