Distributions of absolute ellipticity changes (top) and position angles twists (bottom) for the observed and hydro-simulated sample. The left panels summarize changes between 0.25″ and the Einstein radius, and the right panels focus on changes between one and two Einstein radii. The observed sample, using the light of nearby galaxies analyzed by Kormendy et al. (2009; green), is compared to the hydro-simulated sample using the mass of the EAGLE hydrodynamical simulations from Mukherjee et al. (2018; blue). The light profiles associated with the simulated galaxies (orange) is also displayed to facilitate comparison between the two samples.