The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated, bright central bulge which gradually fades into a more diffuse halo. The color profile suggests an older stellar population, particularly within the central region, shifting towards redder hues. There is little evidence of spiral arm structure or significant dust lanes. The overall appearance indicates a quiescent system, potentially with a low star formation rate. The galaxy appears relatively undisturbed, with no apparent signs of major mergers or tidal interactions.
