The galaxy presents as a relatively compact structure. It appears to be an early-type galaxy, likely an elliptical or lenticular. The light is dominated by older stellar populations as is evidenced by the reddish-yellow hue. The galaxy's structure lacks any obvious spiral arms or significant dust lanes. There is no distinct bulge or disk. The outer edges fade smoothly into the background sky, which suggests a relatively smooth light distribution. There are no visible signs of any major mergers.
