The galaxy presents as a spiral type, exhibiting a distinct disk structure that is not edge-on but rather observed at an angle closer to face-on. The spiral arms appear loosely wound and are observable, with what appears to be at least two prominent arms emanating from the central region. The arms show variations in brightness, indicating regions of differing stellar populations or dust obscuration.

The central bulge is not dominant, appearing relatively small compared to the overall disk size. There is no clear presence of a strong bar feature. The overall colour suggests that the galaxy may be actively forming stars, particularly within the spiral arms, and this may be more prominent on one side.

There is evidence of some gravitational disturbance, either in the form of asymmetries in the disk or tidal features. This suggests a past or ongoing interaction with another galaxy, possibly a minor merger or close passage. Alternatively, this could be an example of an irregular galaxy due to the non-symmetric shape, not of a spiral galaxy. There is an extended halo of material surrounding the main body of the galaxy.