The galaxy presents as a relatively smooth, elliptical-like structure. The central region exhibits a high surface brightness with a slightly blue hue, suggesting a potentially older stellar population. The overall shape is elongated, with a cigar-shaped appearance. There is no obvious evidence of spiral arms or significant dust lanes. The outer regions of the galaxy fade gradually into the background, exhibiting a diffuse halo. There is no obvious evidence of a recent major merger or significant tidal disturbances.
