The galaxy presents a generally smooth and rounded morphology. The central region exhibits a high degree of luminosity, appearing as a bright, concentrated bulge with a yellow-white hue. Moving outwards from the core, there's a gradual decrease in surface brightness. The outer regions of the galaxy possess a less defined structure, appearing somewhat diffuse. Faint disk-like features may be present, but their visibility is low, and the galaxy lacks prominent spiral arms or bars. The overall color appears to be relatively red, suggesting a population of older stars and a low rate of star formation. There appear to be no signs of any major mergers occurring, but a minor disturbance could be occurring.