The galaxy presents as a spiral type, exhibiting a prominent disk structure. The disk is not perfectly edge-on, as evidenced by the slight visibility of the central bulge region.

Spiral arms are clearly discernible, appearing somewhat tightly wound around the central bulge. These arms exhibit a clumpy structure, indicative of active star-forming regions. The bluer hue of the spiral arms suggests the presence of a young, hot stellar population. While difficult to resolve distinctly, the galaxy likely has 2-3 spiral arms.

The central bulge region displays a smoother texture and a slightly more concentrated luminosity, characteristic of older stellar populations. The bulge is moderate in size relative to the disk. There is no evidence of a strong bar feature.

Overall, the galaxy appears relatively undisturbed, displaying a regular spiral morphology with no major signs of recent mergers or tidal interactions, although a minor disturbance cannot be ruled out.
