The galaxy appears to be a spiral galaxy, exhibiting a prominent disk structure. The spiral arms are well-defined, showing a winding pattern that transitions from tightly wound to more open as they extend outward from the galactic center. There is evidence of a moderate bulge in the central region, though it is not the dominant feature. The galaxy is not perfectly edge-on; we observe it at an angle, providing a clear view of the spiral structure. The overall color suggests ongoing star formation, with bluer regions in the arms and a yellower central bulge. There might be a weak bar feature present across the central bulge. The galaxy appears relatively isolated, with no obvious signs of major interaction or merging events. It is likely a mature spiral galaxy with a mix of stellar populations and ongoing star formation processes.
