The galaxy appears as a relatively smooth, elliptical object. Its core exhibits a yellowish hue, suggesting an older stellar population. The light gradually fades outwards from the center, with a slight elongation along one axis, deviating minimally from a perfect circle. There is no visible evidence of spiral arms or significant dust lanes. It is likely a fairly massive galaxy, with relatively low star formation activity. There may be some evidence of a minor disturbance, but the structure appears to be largely undisturbed.
