The galaxy appears as a centrally concentrated system with a smooth, somewhat elliptical morphology. The central bulge exhibits a yellowish-white hue, suggesting an older stellar population. Moving outward from the core, a subtle color gradient is observed, transitioning toward a slightly bluer shade. The outer regions show hints of a faint, diffuse disk. There are no obvious signs of significant dust lanes or spiral arm structure. The galaxy appears relatively undisturbed, with no prominent tidal features or evidence of a major merger event. The overall appearance indicates a galaxy with a moderate mass and a low star formation rate.
