The galaxy presents as a spiral galaxy with a prominent disk structure. The spiral arms are well-defined but exhibit a flocculent, or patchy, morphology. The arms appear to be tightly wound in the inner regions, transitioning to a more open pitch angle at greater radii from the central bulge. The central bulge is relatively small and concentrated, appearing roughly spherical and exhibiting a smooth, yellow-orange color, likely indicating an older stellar population. There is a hint of a bar-like structure but it's weak. The overall color of the disk is a mix of blue and green hues, suggesting ongoing star formation within the spiral arms. The galaxy's morphology is generally undisturbed, showing no strong signs of major interaction or merging events.
