 This image from Hubble, released in May 2022, shows the barred spiral galaxy NGC 7496, which lies over 24 million light years away. The spiral arms extend from a distinct bar that crosses the center of the galaxy. These bars are thought to be regions of rich star formation as gas is channeled inward towards their centers. It was expected that Webb was going to clearly see star clusters in the hearts of these dense molecular clouds that Hubble cannot see. As we transition to the web view, we can see that it still picks up the glowing gas, but also shows much more detail. In Hubble's image, the galactic nucleus is just a bright, featureless glow. Webb cuts through and shows much greater detail about what's happening in the space around the supermassive black hole around which the galaxy revolves.