The galaxy presents as a spiral type, exhibiting a pronounced disk structure. Two distinct spiral arms are clearly visible, emanating from a central bulge. These arms appear loosely wound. There is a suggestion of flocculent structure within the arms. The bulge presents with a moderate size. Overall color indices suggest a galaxy with ongoing star formation. There might be weak indications of a bar-like structure crossing the central region. Possible signs of minor gravitational disturbance within the spiral arms are present, though no major merger is apparent. The majority of light emanates from the disk component rather than the bulge.
