The galaxy presents as a single, luminous entity with a fairly smooth overall structure. It appears roughly elliptical with a color gradient moving from a yellow-white central region to a bluish halo. There is no obvious spiral arm structure or bar visible. The light appears to be fairly concentrated towards the center, suggesting a substantial bulge or a centrally-dominant population of older stars. The outer regions appear more diffuse, potentially indicating a larger radius. There are no obvious signs of major disturbances.
