The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a near-circular morphology, with a smooth light distribution, possibly indicating an elliptical or lenticular type. There is a clear central bulge that displays a yellowish-orange hue, suggesting an older stellar population. The outer regions of the galaxy exhibit a faint, diffuse halo with a bluer coloration. This suggests the presence of a younger population of stars in the outer regions. There are no apparent signs of spiral arms or significant dust lanes. Close inspection reveals no indications of major mergers or tidal disturbances.
