The galaxy presents as a system with a prominent central bulge. The bulge exhibits a smooth morphology and a yellowish-white color, suggesting a population of older stars. Extending from this central region is a discernible disk component, which is not quite as prominent as the bulge. The color gradients within the disk are more varied. There is evidence of possible disruption of the disk, or perhaps tidal features suggesting a past interaction. The disk shows both reddish tones along one side and bluish tones along the other. It's unclear if there is an active galactic nucleus. The overall shape is somewhat elliptical, but also disturbed.
