Decomposition of HE 1029-1831 with Budda. We show (from left to right) the original K-band ISAAC-image, the Budda-model, and the residuum obtained by division galaxy/model. Here, blue indicates that the original image has more flux than the model while red indicates that the model has more flux than the original image. In the lower row, we show an elliptically averaged radial profile of the galaxy, the single components, and the model. Next to it, we show the difference galaxy-model, ellipticity, and position angle.