The galaxy presents as a spiral type, exhibiting a relatively well-defined disk structure. The arms appear open and loosely wound. A central bulge is visible, with a size that appears to be moderate in proportion to the disk. Two spiral arms are clearly visible. There is evidence of ongoing star formation within the arms, suggested by their patchy texture. The disk is seen face-on. There is morphological disturbance, suggesting a possible gravitational interaction with a smaller satellite galaxy or recent merger event.
