The galaxy appears to be an edge-on spiral galaxy, exhibiting a flattened, disk-like morphology. A prominent dust lane bisects the galaxy's mid-plane, obscuring light from the galactic center. The bulge component is not distinctly boxy or rounded. Evidence of recent major or minor merger activity is not visually apparent. 

The overall color profile suggests the presence of both older stellar populations, indicated by yellowish hues in the central regions, as well as younger, bluer stars primarily located in the outer disk. Patches of red are distributed non-uniformly in areas within the disk. These features suggest ongoing star formation within the galaxy.
