The galaxy exhibits a morphology consistent with a spiral or disk galaxy seen nearly edge-on. There is a central bulge, appearing yellowish, indicative of an older stellar population. The disk component displays a bluer color, suggesting the presence of ongoing star formation. A distinct asymmetry is observed along the disk, potentially indicating a gravitational interaction or tidal disturbance. There appears to be a more tightly wound spiral arm or concentration of stellar mass on one side and a more diffuse stellar distribution on the other.
