This galaxy presents as a spiral type, exhibiting well-defined arms emanating from a central bulge. The arms display a tightly wound morphology, suggesting a relatively high shear rate within the galactic disk. A strong central bulge is not apparent. Patches of star forming regions are interspersed throughout the spiral arms. The galaxy appears to be isolated, showing no clear signs of major interaction with other galaxies. There may be some minor irregularities or disturbances in the outer disk, but overall the disk structure appears relatively undisturbed. A bar structure is not apparent, but could potentially exist given the viewing angle.
