The galaxy presents as a spiral type, showing a prominent disk structure. Its arms exhibit a moderate winding, showing an intermediate pitch angle. Indications suggest a three-armed spiral structure, with asymmetry in the arm morphology and luminosity. A distinct central bulge is observed, with an apparent bar feature cutting through the bulge region. The bulge's size appears to be moderate relative to the overall disk. Some regions of enhanced star formation are visible within the spiral arms, appearing bluer in color. Overall, there is an impression of minor disturbances to the galaxy's structure.
