The galaxy presents as a spiral type with a notable disk structure. Two prominent spiral arms are visible, exhibiting a loose winding pattern. There appears to be a moderate bulge component at the galactic center. The galaxy exhibits signs of recent or ongoing star formation, as evidenced by the blue hue within the spiral arms. The overall morphology suggests a system that is relatively undisturbed, although subtle irregularities in the arm structure could indicate minor gravitational interactions or internal dynamical processes. The system does not appear to be undergoing a major merging event. The color gradients across the disk suggest varying stellar populations, with bluer, younger stars concentrated within the spiral arms, and redder, older stars likely populating the bulge and inner regions.
