The galaxy presents a spiral morphology, exhibiting a prominent disk structure. Spiral arms are clearly visible, appearing somewhat tightly wound. They originate from the central bulge and extend outwards. The central bulge appears relatively small. The galaxy displays a moderate degree of inclination relative to our line of sight. Color gradients are apparent, with a yellowish hue concentrated in the central bulge, suggesting an older stellar population, and bluer tones present in the outer spiral arms, potentially indicative of younger, hotter stars and ongoing star formation. Overall the galaxy does not show evidence of major disturbances or ongoing mergers. There is a suggestion of a bar structure present, but it is weak.