Comparison of inferred galaxy intrinsic shape parameters for our modelled galaxies. The galaxy sample is divided into Fornax3D LTGs and ETGs (squares), SAMI passive galaxies (stars) and ATLAS^3D ETGs (circles). Also added as diamonds are the massive lensed ETG ESO286-G022 by Poci & Smith (2022), FCC 47 by Fahrion et al. (2019) and Thater et al. (in prep.), PGC 046832 by den Brok et al. (2021), which is also discussed in Sect. 4, and the three simulated LTGs by Zhu et al. (2020), which are discussed in Sect. 5. Both the intrinsic intermediate-to-major axis ratio p (left panel) and minor-to-major axis ratio q (right panel) show no significant change for the majority of the galaxies. There is no clear trend of increasing discrepancy with galaxy morphology or triaxiality T ≡ (1 − p²)/(1 − q²). Uncertainties were calculated by including all models within of the best-fit model.