The galaxy appears as a centrally concentrated, relatively symmetrical object. It presents a generally smooth morphology, with little evidence of spiral arms or significant substructure. The light distribution is heavily dominated by the central bulge or core, which shows a bright concentration. There is a color gradient within the galaxy, transitioning from a bluer hue towards the inner regions and shifting towards redder colors outwards, suggesting a gradient in stellar populations. A small amount of disturbed matter is visible in the arms.
