The galaxy presents as a disk galaxy, viewed at a significant angle, but not quite edge-on. A central bulge is apparent, although it does not dominate the galaxy's overall structure. There is evidence of spiral arm structure, but the arms are not sharply defined and appear somewhat flocculent. A bar is suspected, based on the somewhat elongated shape of the central bulge.

The galaxy's light is primarily blue-shifted, with a modest amount of red-shifted light visible. The object is likely undergoing some star formation, though at a moderate rate.

There is evidence of disturbance in the overall morphology, suggesting potential interactions with nearby galaxies. The disturbances seem major, with a possibility of merging having occurred or currently in progress. Overall, the galaxy appears as a disturbed spiral with ongoing star formation and evidence of significant interactions.
