The galaxy presents a distinct spiral morphology. Two prominent spiral arms emanate from a central bulge. The arms exhibit a moderate winding, not tightly coiled nor loosely extended. They appear somewhat fragmented, suggesting ongoing star formation regions. The bulge contributes noticeably to the overall light profile, though it does not dominate the galaxy's luminosity. There's a hint of a bar-like structure bisecting the central region. No major signs of a recent or ongoing merger are apparent, though subtle disturbances may be present within the arm structure, potentially indicating minor interactions. The galaxy is observed at a significant redshift, implying a considerable distance. The disk is viewed face-on, allowing for a clear view of its spiral structure.
