The galaxy presents a complex morphology, exhibiting characteristics of a spiral structure that is undergoing a possible merging event. It is observed at a slight angle relative to edge-on, revealing a disk-like structure. The central region displays a moderate bulge. A distinct arm appears disrupted or fragmented on the left side of the galaxy. The light is not smooth but rather uneven. Blue hues are prominent, indicating the presence of recent star formation activity within the galactic arms. The disk appears clumpy. There may be evidence of tidal tails indicating a recent merger. Dust lanes are not prominently visible.
