The galaxy presents as a roughly elliptical, smoothed structure. There is no evident spiral arm structure or disk. The central region exhibits a bright, concentrated core that fades into a less luminous halo. Color gradients are subtle, but there's a hint of redder tones in patches within the brighter core that may indicate older stellar populations. The overall color appears to be slightly bluer toward the outer edges, potentially suggesting ongoing, low-level star formation in the periphery. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions.
