This galaxy presents as a relatively smooth, elliptical system. The core region exhibits a high degree of central concentration and a bright, yellowish-white hue, suggestive of an older stellar population. The outer regions show a gradual decrease in surface brightness with a subtle transition in color, becoming slightly redder. There is little evidence of spiral arm structure or significant dust lanes. The overall morphology indicates a relaxed system that has likely undergone significant dynamical evolution. Although the image does not reveal prominent features indicative of a recent major merger, the faint, disturbed features in the outskirts suggest a potential minor disturbance. The galaxy displays an almost perfectly round shape.
