Image 1 (top left): The first image was captured in the visible spectrum, as we would see it with the naked eye.

Image 2 (bottom left): In the second image, an inverse filter was applied to better highlight the comet’s broad, visible tail.

Image 3 (right): In the third image, a Larson–Sekanina filter was applied, allowing the comet’s ejection jets to be observed — material expelled during its rotation which, as it sublimates (changes directly from solid to gas), contributes to the formation of its characteristic tail.