The galaxy presents as a spiral type, possessing discernible spiral arm structures emanating from a central bulge. The arms appear moderately wound, exhibiting a predominantly two-armed structure. The arms display a somewhat flocculent morphology. The central bulge appears to be of moderate size relative to the overall galactic disk. There is faint evidence of a bar-like feature. The galactic disk is not perfectly face-on, showing a slight inclination. There are no obvious signs of major mergers or significant tidal disturbances, although some minor irregularities within the spiral arms suggest the possibility of minor interactions or internal dynamical processes. The galaxy is characterized by active star formation as indicated by the blueish color of the spiral arms.
