Notes. Rest-frame IR luminosities (8–1000 μm) and corresponding SFRs were derived from IRAS 60 and PACS/IRAS 100 μm fluxes. The uncertainties of L_IR and SFRs are ∼0.12 dex and ∼0.3 dex, respectively. For J1100 and J1152, the PACS 70 μm fluxes were used as a proxy for the 60 μm flux. For J0232 there are no FIR data, but we estimated them by scaling the WISE+PACS spectral energy distribution (SED) of J1152 (also a red ETG) to the WISE SED of J0232. Stellar masses were calculated from 2MASS XSC K-band magnitudes, as described in the text. J1010 and J1100 show K-band excesses that might be indicative of an important contribution from AGN-heated dust (see Jarvis et al. 2020 and Shangguan & Ho 2019, respectively) and thus, for them we used J-band magnitudes instead. Indeed, in the case of J1100, we use M_* from Shangguan & Ho (2019), converted to our cosmology. Columns from 5 to 10 list the isophotal major and minor axis at 25 mag arcsec⁻², position angle (PA) and inclination (i) from r-band SDSS DR6 photometry (2007). Morphological classifications come from visual inspection of the SDSS images shown in Fig. 1 and from the Galaxy Zoo 2 project (Willett et al. 2013).