The galaxy exhibits a spiral morphology, appearing as a disk-shaped system with a prominent central bulge. The spiral arms are clearly discernible, though not tightly wound. The arms appear to be somewhat fragmented, with varying degrees of star formation activity indicated by the mottled blue regions along the spiral arms, implying ongoing or recent bursts of star formation. The central bulge is yellowish, which suggests an older stellar population. There's a hint of a bar-like structure crossing the central region of the galaxy. Overall, the galaxy appears relatively undisturbed, showing no significant signs of major merger activity, but potentially a minor disturbance.