The galaxy exhibits a flattened, disk-like morphology, suggesting it is a spiral or lenticular galaxy viewed at a considerable inclination. A central bulge is visible, appearing yellowish in color, indicating a population of older stars. The disk shows some evidence of spiral arm structure. The overall color gradient suggests ongoing star formation within the disk, though the bulge appears quiescent. There is some indication of possible disturbance in the outer regions of the disk, but it could be an effect of imaging quality. 
