The galaxy exhibits a clear spiral morphology, displaying prominent spiral arms. The arms appear loosely wound, extending outwards from a central bulge. The bulge itself seems relatively small in proportion to the disk. There is evidence of ongoing star formation within the spiral arms, indicated by the presence of bluer regions. The galaxy appears largely undisturbed, although a close inspection could reveal minor tidal features hinting towards a past interaction. The galaxy is observed at a redshift, indicating its distance and the expansion of the universe. The orientation of the galaxy is somewhat tilted relative to our line of sight, offering a perspective of the spiral structure. Overall, the galaxy presents a well-defined spiral structure with active star formation in its arms.
