The galaxy presents as a spiral type, with a notable disk structure. The spiral arms are well-defined and appear tightly wound. A central bulge is discernible, exhibiting a moderate size relative to the disk. The bulge appears less blue than the disk. There is evidence of active star formation throughout the disk, particularly concentrated within the spiral arms.

Distortions are visible in the morphology. One arm seems disconnected from the central bulge. This could indicate a minor interaction with another galaxy or another form of disturbance. 
