The galaxy presents a generally smooth and rounded morphology. The central region exhibits a bright, concentrated luminosity, indicative of a significant stellar population, possibly an active galactic nucleus or a dense bulge. Moving outwards from the core, the light gradually diffuses, suggesting a less concentrated stellar density in the outer regions. There are subtle color variations across the galaxy, with the core appearing slightly yellower compared to the bluer hues in the surrounding halo. These color differences could reflect variations in stellar population ages, metallicities, or dust content. There is some minor evidence of disruption, but the overall structure appears relatively undisturbed, showing no signs of major mergers.
