The galaxy presents as a largely smooth, elliptical-like structure. There is a concentration of light toward the center, suggesting a prominent galactic nucleus. The light smoothly dissipates outwards towards the edge of the galaxy. There is a subtle color gradient, with the central region displaying a yellow-orange hue, subtly shifting toward a paler yellow. No distinct spiral arm structures or dust lanes are visible within the observable morphology. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. Based on the galaxy’s morphology, it appears to be an early-type galaxy, perhaps with ongoing star formation. The angular roundness implies no extreme flattening. It is possible there is a small amount of disk.
