The galaxy presents as a spiral type, exhibiting a discernible disk structure. Spiral arms are apparent, predominantly featuring a two-arm morphology with tight winding. The central bulge appears moderate in size and luminosity relative to the overall disk. Some of the spiral arms appear flocculent, with indications of active star formation regions evidenced by their bluish hue. The galaxy is not viewed edge-on, allowing observation of its spiral structure. There is no obvious evidence of a strong bar structure. No significant merging or major disturbances are noted, although minor asymmetry in the spiral arms suggests possible past interactions or ongoing internal processes.