The galaxy presents a distinct spiral morphology, viewed at a moderate inclination, but not quite edge-on. Spiral arms are visible and traceable within the disk. There's a suggestion of ongoing star formation, indicated by the bluish hues within the spiral arms. The central bulge appears relatively small or non-existent, with the disk dominating the overall structure. There's a faint suggestion of a bar structure bisecting the galaxy. The galaxy also displays characteristics indicative of potential tidal interactions or mergers. There is a clear asymmetry to the overall shape, and some visual disturbances in the disk. These disturbances could be indicative of ongoing or recent interactions with smaller galaxies.
