The galaxy appears to be a relatively smooth, elliptical system. It exhibits a concentrated, bright central bulge that transitions smoothly into a diffuse halo. There is a distinct color gradient, with the core region displaying a yellowish-white hue, indicative of an older stellar population. The outer regions of the galaxy are fainter, showing a slightly bluer color, possibly due to a small amount of ongoing or recent star formation in the outer parts. There is no indication of a prominent disk structure or spiral arms. The overall morphology suggests a relatively evolved galaxy with a high degree of spherical symmetry and minimal signs of recent major merger activity. There may be some indication of minor gravitational disturbance in the system, but no major disruption is evident. 
