Radial profiles of asymmetric galaxies from the Raj et al. (2019) LTG sample. These galaxies are within the virial radius of the main Fornax cluster and are clearly asymmetric in some form (see text for details). In all cases, our default radial profile derivation permits the identification of an edge feature in the colour or density profiles (vertical dashed line). However, as we are using fixed elliptical annuli, our profiles should be considered as an average representation of the data.