This galaxy appears to be a spiral galaxy, exhibiting a discernible disk structure with prominent spiral arms. The arms seem somewhat flocculent, displaying a patchy distribution of star formation regions.

The galaxy possesses a central bulge which is moderate in size. The bulge region appears smoother and more uniformly colored compared to the disk, suggesting a more evolved stellar population.

There is no obvious presence of a strong bar structure. While some asymmetry is present in the disk, no obvious tidal distortions or signs of recent major merger activity are noted. This suggests the galaxy is relatively undisturbed in its recent evolutionary history, though minor interactions cannot be ruled out.

Overall, the galaxy appears to be a fairly normal spiral galaxy, viewed at a slight angle relative to edge-on.
