The galaxy appears as a relatively smooth, elliptical structure. It exhibits a concentrated central bulge, characterized by a yellowish-orange hue, indicating an older stellar population. The light tapers off gradually towards the outer regions. There is a slight elongation, departing from a perfect circular shape, trending more towards an in-between structure. No distinct spiral arms or prominent dust lanes are visible. There may be some minor disturbance in morphology but it is otherwise not undergoing a major merger. The galaxy is at a considerable distance, as evidenced by its redshift.
