A perfect pair! In this image, @NASAWebb and @NASAHubble team up to show unique details of galaxy pair VV191. Webb provides a view in near-infrared light, while Hubble shows ultraviolet and visible light wavelengths. Webb’s new data allowed us to trace the light that was emitted by the bright white elliptical galaxy, at left, through the winding spiral galaxy at right – and identify the effects of interstellar dust in the spiral galaxy. Image description: The background of this image is black. Two large, very bright galaxies dominate the center of the image. The elliptical galaxy at left is extremely bright at its circular core, with dimmer white light extending to its transparent circular edges. At right is a bright spiral galaxy. It also has a bright white core, but has red and light purple spiral arms that start at the center and turn clockwise going outward. They end in faint red and appear to overlap the elliptical galaxy at left. Throughout the scene are a range of distant galaxies, the majority of which are very tiny and red, appearing as splotches. Credit: NASA, ESA, CSA, STScI, R. Windhorst (Arizona State University), W. Keel (University of Alabama), S. Wyithe (University of Melbourne, Australia), and the JWST PEARLS Team