The galaxy presents as a spiral type, exhibiting a distinct disk structure. The spiral arms are prominent, loosely wound, and appear to be fairly symmetric. Two clear arms emerge from a central bulge region. There is a hint of a bar-like structure crossing the central bulge, though it appears weak and not fully developed. The central bulge itself seems relatively small compared to the overall size of the disk. Patches of blue suggest recent star formation occurring along the spiral arms. There is no indication of any major merging events. The orientation is close to face-on, allowing for a clear view of the spiral structure.
