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Fig. 2.

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Comparison of the aged version of ZF-UDS-7329 (z = 3.2) and the massive relic galaxy NGC 1277 (z = 0). The inset images of ZF-UDS-7329 and NGC 1277 are from the F444W (JWST) and F814W (Hubble Space Telescope) filters, respectively. The remarkable similarity between the two spectra is evident, and the major differences appear in important absorption features, such as the CN bands, Mg, and Na doublet lines. This is likely due to the particular chemistry of NGC 1277 and the continuum systematics on its observed spectrum.

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