The galaxy exhibits a clear disk structure, with spiral arms that appear tightly wound. The arms are somewhat difficult to discern clearly; there may be more than four. The central bulge is small and not particularly prominent, with a yellow hue, suggesting an older stellar population in this region. The disk appears to be viewed at an angle, with some dust lanes visible, especially near the edges of the disk. The overall shape is elongated, implying an inclination relative to our line of sight. The galaxy displays signs of active star formation, particularly in the spiral arms, where there are faint blue regions. No strong evidence of a bar structure is apparent. There is no obvious signs of a major merger, but some minor asymmetry indicates a possible disturbance in the galaxy's history.
