The galaxy presents a largely smooth, rounded morphology. There is a bright, concentrated central bulge that appears to be roughly spherical. Fainter diffuse light extends outwards from the core, forming a halo or envelope. The colour of the central region is predominantly yellow, indicating a population of older stars. The outer regions of the galaxy exhibit a slightly bluer tinge, possibly suggesting younger stellar populations and ongoing, but low-level star formation. There is no obvious evidence of spiral arms or a pronounced disk structure. Additionally, there are no obvious signs of a major merger event, tidal tails, or significant dust lanes, though minor disturbances cannot be ruled out based on this image.
