The galaxy presents as a spiral type, with a notable disk structure viewed at a slight inclination. The central bulge appears relatively small and indistinct from the disk. A bar structure is not clearly visible. The spiral arms exhibit a tightly wound morphology, displaying a multi-armed pattern with some segments appearing less defined. The overall color suggests ongoing star formation, with a greater concentration of older stellar populations in the nuclear region. There is no obvious sign of a major merging event. The galaxy appears as a relatively undisturbed system.
