The galaxy appears as a centrally concentrated object with a diffuse, extended halo. The core region exhibits a yellowish-white hue, suggestive of an older stellar population. There is an overall lack of distinct spiral arm structure or prominent dust lanes. The halo shows a more subtle bluish tint in the outer regions, possibly indicating the presence of some younger, bluer stars. The object's shape is somewhat elliptical, with a moderate degree of elongation. The overall impression is of a relatively smooth, evolved galaxy undergoing limited recent star formation, and without any signs of ongoing major merger activity.
