The galaxy presents as a spiral with a prominent central bulge, surrounded by a disk that exhibits distinct spiral arm structures. The arms appear relatively tightly wound. There is evidence of a bar feature crossing the central bulge. The luminosity profile suggests a centrally concentrated morphology, with light diminishing gradually toward the outer regions. The galaxy exhibits a smooth, coherent structure, showing no signs of ongoing major merger activity. The morphology is consistent with a relatively undisturbed spiral galaxy.
