The galaxy presents as a somewhat elliptical, though not perfectly round, structure. A bright, concentrated central bulge is clearly visible, suggesting a high stellar density in the core. The outer regions appear fainter and more diffuse, with a slightly bluer color than the central bulge, which is more yellow. This difference in color could indicate younger star formation in the outer regions compared to the older stellar populations in the bulge. Overall, the galaxy appears relatively undisturbed, with no obvious signs of ongoing major mergers or tidal distortions. However, there is a faint, subtle asymmetry to the galaxy's shape, which could be due to a minor interaction or internal dynamics.
