The galaxy presents as a single, relatively smooth object with a centrally concentrated light profile. It appears elliptical in shape, displaying a high degree of roundness. There is a gradual decrease in luminosity from the core outwards, lacking distinct spiral arm structures or significant dust lane features. Color gradients are subtle, with a slightly yellower core transitioning to a bluer halo. No major disturbances or signs of ongoing merger activity are readily apparent within its structure.
