The galaxy presents a spiral morphology, displaying well-defined spiral arms. These arms exhibit a somewhat flocculent structure, lacking continuous, sharply defined boundaries. A central bulge is present, though it appears relatively subdued compared to the overall size of the galactic disk. The bulge shows a yellowish hue, suggestive of an older stellar population. The spiral arms appear bluer in color, indicating ongoing star formation. No prominent bar structure is evident. There is a possible interaction or minor disturbance visible, perhaps suggesting an ongoing merger, but it is subtle and not highly disruptive to the overall structure. Overall, it appears to be a relatively normal spiral galaxy, undergoing active star formation within its arms.
