The galaxy appears as a centrally concentrated object with a smooth, diffuse halo. The core exhibits a bright, yellowish-white color, suggesting a population of older stars. The outer regions display a gradual decrease in luminosity, fading into the background sky. There is a very subtle elongation, but overall the galaxy appears relatively symmetrical. No distinct spiral arm structures or significant dust lanes are apparent. The overall color gradient indicates a potentially passive or quiescent stellar population. It is likely an early-type galaxy, based on its apparent morphology. There is little evidence of ongoing major mergers or tidal disturbances.
