The galaxy presents as a spiral type, possessing a noticeable disk structure. Spiral arms are clearly visible, exhibiting a somewhat flocculent morphology. The arms appear relatively tightly wound. A central bulge is present, appearing moderately sized relative to the overall galactic disk. The bulge exhibits a yellowish hue, indicative of an older stellar population. The disk component displays a bluer color, consistent with ongoing star formation. There is no obvious strong central bar structure, although a subtle, weak bar might be present. The overall appearance of the galaxy suggests it has not undergone any recent major merging events, though some minor disturbances may be present as the spiral arms seem slightly disrupted. The galaxy is inclined relative to our line of sight, but not edge-on, allowing clear observation of the spiral structure.
