1. Introduction

2. Methods
2.1. Data description
2.2. Red sample selection and morphological classification
2.3. GALFIT modelling and PSF correction
2.4. Surface brightness profiles
2.5. Photometric corrections
2.6. Elbow: automated break analysis of disc surface brightness profiles
2.7. Efficiency and reliability of the PSF correction
2.8. AGN in the initial sample

3. Results and discussion
3.1. Statistics of the red galaxy sample by morphology
3.2. Star formation rates and masses as a function of the morphology
3.3. Types of disc profiles in the S0 sample
3.4. Comparison of anti-truncated discs of S0 galaxies at 0.2<z<0.6 with local analogs
3.5. Effects of the PSF on the profiles

4. Conclusions