The galaxy presents as a somewhat smooth, elliptical structure. The central region exhibits a bright, concentrated luminosity, indicative of a high stellar density. This core is yellowish in color, suggestive of an older stellar population. Moving outwards from the core, the intensity of light decreases gradually. The outer regions appear slightly more diffuse and reddish, potentially due to the presence of dust or a slightly younger stellar population compared to the core. There is a hint of a disk-like structure, but the smoothness is dominant. No distinct spiral arms or significant dust lanes are discernible. The galaxy appears relatively undisturbed, without any major signs of recent mergers or tidal interactions. The overall form leans towards being somewhere between round and elliptical, but the object is definitely not cigar-shaped.
