The galaxy presents a generally smooth and rounded morphology. It displays a central bulge that appears significantly brighter than the surrounding regions. There is a subtle color gradient, transitioning from a slightly bluer hue in the inner regions adjacent to the bulge, to a redder tint at the outer edges. The disk shows little or no discernible spiral arm structure or prominent dust lanes. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal disruptions. The overall structure suggests a galaxy that is dominated by older stellar populations, particularly in the outer regions, with signs of continued star formation, or a younger stellar population in the inner parts.
