The galaxy presents a largely smooth and rounded morphology. It exhibits a concentrated central region that appears relatively bright, transitioning into a fainter, more diffuse halo. The color profile suggests a dominance of older stellar populations, with a yellowish-white hue characterizing the central region. There are no readily apparent spiral arm structures or significant dust lanes visible. Subtle color variations might indicate varying stellar densities or compositions within the extended halo. The overall appearance suggests a system that is fairly undisturbed and well-mixed.
