The galaxy presents as a disk galaxy with a well-defined spiral structure. The spiral arms are loosely wound, extending outwards from a somewhat subdued central bulge. Two prominent arms are clearly visible, though the presence of additional arms cannot be ruled out due to image clarity. There is evidence of on-going star formation, indicated by the bluish tint within the spiral arms, suggesting the presence of young, hot stars. The galaxy appears to be undergoing some form of interaction or disturbance. This is indicated by the clumpy and distorted appearance of its spiral arms. There may be some indication of a weak bar feature bisecting the central region. The bulge component is relatively small compared to the overall disk size, suggesting a disk-dominated morphology.
