The observed galaxy presents a flattened, disk-like morphology with a moderate inclination relative to the line of sight. A central bulge is visible, appearing relatively bright and concentrated. The disk component exhibits a smooth, somewhat amorphous structure with hints of spiral arm features. Faint color variations are present across the disk. There appears to be a minor disturbance or some asymmetry in its structure, and it is possible that it is undergoing a minor merger. The overall color suggests a mix of stellar populations, with both older, redder stars and younger, bluer stars contributing to the observed light.
