The galaxy appears as a concentrated, elliptical-like structure with a smooth, diffused profile. Its core exhibits a strong, centralized luminosity, suggesting a high stellar density or potential active galactic nucleus. The overall color is redder, consistent with an older stellar population and a low rate of current star formation. No prominent spiral arms or distinct dust lanes are discernible. The galaxy appears relatively undisturbed, lacking any significant signs of ongoing mergers or tidal interactions. Its shape leans towards a moderately elliptical morphology, not perfectly spherical or highly elongated. There is very little disk-like structure visible.
