The galaxy presents as a generally smooth, centrally concentrated object with a somewhat elliptical morphology. The light distribution appears fairly uniform, lacking any distinct spiral arms or bar structure. The core region exhibits a brighter, more intense glow, suggesting a higher stellar density or possible active galactic nucleus. There is faint evidence of some subtle features or irregularities in the outer regions, potentially indicative of minor tidal interactions or internal dynamical processes. The color profile appears relatively homogenous across the galaxy, suggesting a predominantly older stellar population.
