The galaxy presents a complex morphology, appearing as a disk galaxy with a significant bulge component. The disk exhibits a somewhat patchy distribution of luminosity, potentially indicative of spiral arm structures. It's orientation is close to face-on, but seems to be at a slight inclination based on the elongation. The bulge appears moderately sized, contributing a considerable portion of the overall light. The presence of blue colors in the disk might suggest ongoing star formation, particularly within the spiral arm regions. The overall structure doesn't show signs of major disturbances, although the uneven light distribution in the disk could be interpreted as minor interactions or internal asymmetries. There is some evidence that the galaxy possesses spiral arms. There may be a weak bar feature present as well. The light distribution suggests the galaxy is dominated by its disk component rather than the bulge, implying ongoing disk evolution.