The galaxy presents as a single, largely homogenous object with a concentrated central region that appears bright and yellowish. A diffuse halo surrounds the core, displaying a bluish tint. The overall shape of the galaxy is roughly circular. There are hints of possible spiral structure within the disk, but the resolution of the image limits the ability to resolve any distinct arms or features. No major disturbances, strong tidal tails, or evidence of a recent major merger are apparent. There is a low level of ongoing star formation.
