The galaxy presents as a moderately inclined spiral galaxy, with a noticeable bulge component that appears yellowish-white in color, suggesting an older stellar population. The disk exhibits a more diffuse, bluish tint, hinting at the presence of younger, hotter stars and ongoing star formation. 

Spiral arms are faintly visible, appearing somewhat tightly wound around the bulge. There is subtle asymmetry in the spiral arm structure. The dust lanes are also barely visible in the galaxy. The overall structure suggests a galaxy with a relatively ordered morphology, displaying features characteristic of an intermediate spiral type. 

The galaxy's elongated shape indicates a significant inclination relative to our line of sight, and a relatively high concentration of light towards the center of the galaxy.
