The galaxy presents as a relatively smooth, elliptical-shaped object. It exhibits a bright central bulge that gradually fades into the surrounding galactic disk. The color appears to be predominantly white-blue, possibly indicating a population of young to intermediate-age stars. The galaxy is elongated, exhibiting a cigar-like shape. There are no obvious signs of spiral arms or significant dust lanes. Minor disturbances are possibly present. There is no evidence of recent major merger activity or strong tidal distortions.
