The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a generally elliptical morphology, tending toward a rounded shape. There is a distinct color gradient, with a yellowish-white core fading into a bluer, more diffuse outer halo. There is no clear evidence of spiral arm structure or significant dust lanes. The galaxy appears relatively undisturbed, without obvious signs of ongoing or recent major merger events. Some low-level irregular features may be present in the outer regions, though they are not pronounced. The overall impression is of a mature galaxy.
