The galaxy presents as a slightly inclined spiral, potentially exhibiting a barred structure, although this is uncertain. The central bulge appears relatively compact and moderately bright, suggestive of an intermediate stellar population. Disk morphology indicates a degree of irregularity, possibly indicating recent or ongoing interactions. There is a noticeable disturbance to its overall structure, with a hint of tidal features or asymmetric arm structures. The galaxy's color is moderately blue, indicating moderate star formation. The galaxy is not highly concentrated, with a diffuse halo extending beyond the main disk. Overall, the galaxy exhibits characteristics of a transitioning system, likely somewhere between a pure spiral and a more disturbed or potentially merging state.
