The galaxy appears to be a spiral galaxy viewed at an angle. It has a central bulge that is not very prominent, and the spiral arms are loosely wound. The galaxy has a blue hue, suggesting a younger stellar population with ongoing star formation. There is evidence of minor disturbance, possibly due to a past interaction or merger. The galaxy's disk shows some distortion and asymmetry. Overall, the galaxy appears to be relatively undisturbed. There is a faint, diffuse halo surrounding the galaxy.
