The galaxy exhibits a distinct spiral morphology. The central bulge appears relatively prominent and has a smooth, concentrated luminosity profile. Traces of a bar feature may be present in the central region.

Spiral arms are visible, with two dominant arms and possibly hints of additional, fainter arms. The arms appear relatively tightly wound around the bulge. The galaxy displays intermediate colors, with a slightly bluer hue along the spiral arms compared to the more yellow/red central bulge, suggesting ongoing star formation within the arms. There may be some regions of more intense star formation.

The disk is viewed nearly face-on. Overall, the galaxy appears relatively undisturbed, although the spiral arms show slight asymmetry, indicating possible past or ongoing interactions. There may also be some signs of minor disturbances.
