The galaxy presents a generally smooth and rounded appearance. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars or potentially an active galactic nucleus. Moving outward from the core, the light appears to gradually fade. There are hints of a diffuse, extended halo surrounding the central region, although its boundaries are poorly defined. No distinct spiral arms or bar-like structures are discernible. The galaxy appears to be relatively undisturbed, showing no obvious signs of recent mergers or major interactions.
