The galaxy appears as a relatively smooth, elliptical structure. It exhibits a bright, concentrated central bulge, with a more diffuse halo extending outwards. The color gradient suggests an aging stellar population, transitioning from yellow-white in the center to a faint redder hue in the outer regions. There is little evidence of significant spiral arm structure or active star formation within the visible spectrum. The overall morphology suggests a galaxy that is approaching a more quiescent state.
