The galaxy presents a primarily disk-like structure with a discernible central bulge. The spiral arms are tightly wound and somewhat fragmented, exhibiting a clumpy morphology. The bulge appears relatively small, but not insignificant, contributing to the overall luminosity. There is evidence of star formation activity within the disk, indicated by the presence of blueish regions. While no major merger is apparent, minor disturbances or interactions may be present, hinted by the irregularities in the spiral arm structure. The galaxy is not highly inclined, presenting a face-on or near-face-on orientation. No bar structure is immediately obvious. The winding pattern is not clear enough to tell if there are more than 4 arms.
