The galaxy presents as a spiral type, exhibiting a prominent central bulge and a relatively high degree of disk inclination. The bulge appears luminous and concentrated. There is some visual evidence of spiral arm structure, although the resolution limits a precise arm count. The spiral arms appear tightly wound, with most of the arm structure concentrated in the inner region. A degree of asymmetry or disturbance is noted in the disk morphology, possibly due to minor interaction or internal processes. There is no clear indication of a strong bar structure.
