The galaxy appears to be a relatively smooth, elliptical-type galaxy. Its overall form presents a somewhat rounded appearance, with a slight deviation towards a more elongated shape. A bright, concentrated central bulge dominates the galaxy's core, indicative of a high stellar density in that region. The light emitted is primarily redder in the central region and transitions to a bluer hue towards the outer edges, suggesting a possible gradient in stellar populations. There is little evidence of spiral arm structure or dust lanes. The outskirts of the galaxy show some faint features, hinting at possible tidal interactions or minor disturbances. The lack of significant distortions suggests that, if present, these interactions are not major mergers.
