The galaxy presents an elliptical morphology, appearing elongated with a cigar-like shape. It exhibits a relatively smooth structure, lacking prominent spiral arms or distinct features. The core region appears brighter and more condensed, with a diffuse, extended halo gradually fading into the background. The color profile suggests a population of older stars, with a reddish-yellow hue dominating. There is no immediately apparent evidence of major ongoing mergers or significant tidal disturbances, although subtle irregularities may indicate minor interactions or past events. The general form suggests this is likely a very massive galaxy, with a low star formation rate.
