The galaxy exhibits a prominent disk structure with clear evidence of spiral arms. These arms appear relatively tightly wound in some regions and more loosely wound in others. The morphology is indicative of a spiral galaxy, with the spiral structure dominating the overall appearance.

A central bulge is visible, although it does not appear to be excessively large compared to the disk. The brightness distribution suggests a higher concentration of older stars within the bulge region.

There is a suggestion of a bar-like structure present in the central region, although it is not strongly defined. The galaxy does not show signs of major disturbance or ongoing merger activity.
