The galaxy presents a generally smooth and rounded appearance. It appears to be relatively compact with no discernible spiral arm structures. The galaxy's color suggests a population of older stars, with a relatively low rate of ongoing star formation. There is a slight variation in color, with the central region appearing somewhat brighter and bluer compared to the outer edges. This could indicate a concentration of younger stars or a more active galactic nucleus in the core. There are no immediately obvious signs of tidal disturbances or mergers.
