Vegetti et al. discovered a satellite galaxy located around a more distant elliptical galaxy acting as a gravitational lens. They were able to detect the satellite galaxy through its effect on distorting light from a background source, causing detectable "dents and blobs" in the ring of light formed by the main lens galaxy. This satellite galaxy has a mass of about 113 million solar masses, making it one of the lowest-mass satellite galaxies detected so far. The discovery provides evidence that gravitational lensing techniques can be used to find satellite galaxies beyond the Local Group and help test theories of galaxy formation and evolution.