The object in question appears to be a spiral galaxy, though its features are somewhat indistinct. The color distribution suggests the presence of stellar populations of varying ages. The central bulge seems relatively small and compact. The spiral arms are diffuse, and exhibit a clumpy morphology, possibly indicating areas of active star formation. There are minor signs of tidal disruption, and possible minor signs of a merger, or past interaction with another galaxy, as evidenced by faint, extended streams of stellar material. The galaxy is seen at a slight angle. The galaxy appears to be fairly large.
