The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge, indicated by a bright, yellowish-orange hue. There's a gradual fading of intensity from the center outwards, suggesting a decrease in stellar density within the halo. No distinct spiral arm structures or prominent dust lanes are visible. The overall morphology suggests a lack of ongoing major star formation within the galaxy. It appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions.
