The galaxy presents as an elongated, elliptical form. It exhibits a smooth, centrally concentrated light profile with no obvious spiral arm structures or prominent dust lanes. The core region appears brighter and exhibits a yellowish hue, possibly indicating an older stellar population. The outer regions show a gradual decrease in luminosity, with a subtle shift towards greenish tones, possibly indicating the presence of younger stars or ionized gas. The galaxy's overall shape is cigar-like with most of the light concentrated around the center. There is some indication of a minor disturbance within the galaxy, potentially a small merging event.
