The galaxy presents as a relatively small object with a disk morphology. There is evidence of disturbance within the disk. The galaxy exhibits a complex structure with some regions appearing smoother than others. A slightly irregular and asymmetrical shape is visible. There is evidence of some minor disturbance present in the arm structure. There is evidence of a potential companion or tidal tail emanating from one edge of the galaxy. Color gradients suggest differences in stellar populations or dust content across the galaxy.
