The galaxy exhibits a somewhat diffuse morphology. The light is not highly concentrated towards the center, indicating a lower degree of central bulge dominance.

The galaxy appears to exhibit a disturbed morphology. There is evidence suggesting a possible interaction or merger event with another galaxy. Faint tidal features or distortions may be present in the outer regions of the galaxy's disk, though any disturbances are faint.

The color gradients within the galaxy suggest a mixed stellar population. The bluer regions suggest active star formation, and redder regions suggest older stellar populations. There is no evidence of a prominent dust lane.
