The galaxy presents as a largely smooth, centrally concentrated structure. Its overall shape appears nearly circular, with a slight elongation noticeable along one axis. The core exhibits a high degree of brightness, suggesting a dense concentration of stars or an active galactic nucleus. Moving outward from the core, the light intensity gradually diminishes. The color profile indicates a relatively even distribution of light across the visible spectrum, with slight bluer tones in the central region and more neutral tones in the outer reaches. No distinct spiral arms or other prominent features are discernible. Overall, the galaxy appears to be relatively undisturbed, lacking any significant signs of ongoing mergers or tidal interactions. It presents a compact and well-defined morphology.
