The object presents as a spiral galaxy, oriented nearly edge-on from our perspective. There is a prominent central bulge, elongated and exhibiting a yellowish-white hue, suggesting an older stellar population. Faint dust lanes can be seen bisecting the bulge, a characteristic feature of edge-on spiral galaxies. 

The spiral arms are tightly wound and diffuse, appearing primarily along the outer edges of the galactic disc. The arms appear bluish, indicating the presence of younger, hotter stars and active star formation regions. The outer disk shows a flattened morphology, extending a considerable distance relative to the bulge.

There is evidence of a strong central bar structure embedded within the bulge. The overall structure suggests a well-formed spiral galaxy, likely not undergoing any significant mergers or major disturbances.
