The galaxy presents as a largely featureless elliptical system. The light profile is dominated by a smooth, centrally concentrated bulge. The core exhibits a bright, relatively uniform color suggesting an older stellar population. There is evidence of a faint, diffuse disk-like structure surrounding the bulge, but no distinct spiral arms or prominent dust lanes are observed. A slight asymmetry in the outer regions might indicate a minor interaction or past merger event, but it's not immediately apparent if this system is actively merging. Overall, the galaxy appears relatively evolved and quiescent.