The galaxy presents as a flattened, disk-like structure, viewed nearly edge-on. There is a central bulge that exhibits a yellowish hue, suggesting an older stellar population. Along the galactic plane, a distinct blue color gradient is observed, particularly toward the outer edges, indicating active star formation. The disk appears relatively smooth, without any prominent spiral arm structures. The overall morphology suggests a system that is potentially undergoing some degree of star formation. There are no obvious signs of a recent major merger or tidal disruption, although there might be some minor asymmetry or disturbance in the disk.
