The galaxy presents a face-on spiral morphology. Two well-defined spiral arms emerge from the central bulge. These spiral arms are of medium pitch angle, neither tightly wound nor significantly open. The arms exhibit a relatively smooth appearance with some clumpy regions, suggesting ongoing star formation. The central bulge is moderately sized and appears yellowish, indicating an older stellar population. There is no strong bar structure apparent within the galaxy. A small fraction of the light appears to be emanating from a smooth, diffuse component. There are no obvious signs of a major ongoing merger, though subtle disturbances cannot be ruled out. The disk dominates the galaxy's appearance, oriented nearly face-on, as no significant edge-on inclination is observed.