  Planets are like children with each one being unique and special. A better
understanding of their collective properties requires a deeper understanding of
each planet. Here we add the transit and eclipse spectra of hot Jupiter
WASP-74b into the ever growing dataset of exoplanet atmosphere spectral
library. With six transits and three eclipses using the Hubble Space Telescope
(HST) and Spitzer Space Telescope (\textit{Spitzer}), we present the most
complete and precise atmospheric spectra of WASP-74b. We found no evidence for
TiO/VO nor super-Rayleigh scattering reported in previous studies. The transit
shows a muted water feature with strong Rayleigh scattering extending into the
infrared. The eclipse shows a featureless blackbody-like WFC3/G141 spectrum and
a weak methane absorption feature in the Spitzer 3.6 $\mu m$ band. Future James
Webb Space Telescope (JWST) follow up observations are needed to confirm these
results.
