The galaxy presents as a relatively smooth, elliptical object. There is a distinct central bulge that appears yellow-white, indicating an older stellar population. The galaxy exhibits a slight elongation, deviating from a perfectly circular shape, but is closer to round than cigar shaped. There is minimal evidence of spiral arm structure or significant dust lanes, suggesting a lack of recent major mergers. The outer regions of the galaxy fade gradually into the background sky, demonstrating a decreasing stellar density with increasing distance from the center. There is no apparent tidal tail or other indications of ongoing interaction with another galaxy. The overall color is consistent with a galaxy where star formation has slowed or ceased, leading to a population dominated by older, redder stars. The galaxy may contain faint features, but the image quality is low.
