The galaxy presents a somewhat elongated, disk-like morphology with a noticeable bulge. The central bulge exhibits a yellowish hue, potentially indicating an older stellar population. The disk appears bluish, suggesting the presence of younger, hotter stars and ongoing star formation. There is a hint of spiral structure, although it appears somewhat disrupted or irregular. The galaxy appears to be interacting with a smaller companion galaxy nearby, and the overall structure suggests it is inclined at an angle between face-on and edge-on. Dust lanes are either minimal or obscured. The overall light distribution suggests it is dominated by bulge-like profile.
