Example |$rgb$|  JWST CEERS images visually identified by F23 as a disc (⁠|$p_{\rm {disc,F23}}>0.5$|⁠) but with low featured vote fractions in GZ CEERS (⁠|$p_{\rm {feat,GZ}}< 0.3$|⁠); aka apparently featureless discs. We show a representative sample at low redshift (top row; |$0.01 < z < 1.78$|⁠), medium redshift (middle row; |$1.78 < z< 2.44$|⁠), and high redshift (bottom row; |$2.44 < z < 9.26$|⁠). In the top left corner of each image we provide the CEERS ID of the galaxy. In the bottom left corner of each image we provide the GZ featured vote fraction, |$p_{\rm {feat, GZ}}$|⁠, the F23 disc vote fraction, |$p_{\rm {disc, F23}}$|⁠, the Sérsic index fit by F23, |$\rm {n}_F$|⁠, and the HST CANDELS redshift, z, for each galaxy. The examples shown are representative of a sample of apparently featureless discs one can select by combining GZ CEERS with expert classifications and/or parametric morphologies from F23. Note that these are the exact images which were shown to GZ CEERS volunteers during classification; volunteers were asked to classify the galaxy in the centre of the image.