Resumen

We present a multi-wavelength study of the morphology and spectral energy distribution (SED) of the OH Megamaser galaxy (OHMG) IRAS16399-0937, based on new HST ACS broad band (F814W) and emission line (Hα+[NII]) images and archive data from HST, 2MASS, Spitzer, Herschel and the VLA.