The galaxy presents a spiral morphology. It exhibits well-defined spiral arms, showing a dual-arm structure, with moderate winding. A central bulge appears prominent, though not entirely dominant.

There is no apparent edge-on disk structure, and the galaxy is viewed at an angle. No significant bar feature is observed crossing the central bulge.

Within the spiral arms, the colour distribution implies the potential for ongoing star formation, though the intensity is generally low. The light emitted is redder towards the central bulge, suggesting an older stellar population there. There are indications of a spiral morphology, with a dual-arm structure, moderate winding, and only weak signs of ongoing star formation.

No obvious signs of strong tidal disturbance or a major merger are readily apparent from the image.
