The discussion centers on the theoretical shapes of black holes, specifically their event horizon topology. It is noted that stationary black holes in four-dimensional spacetime typically have a spherical event horizon, while rotating black holes exhibit an oblate ellipsoid shape. The concept of singularities is debated, with the understanding that they are theoretical constructs rather than physical realities, and improved models aim to eliminate them. The event horizon is crucial in defining the shape of a black hole, as it represents the boundary of the entity, while the interior structure remains largely undefined in classical theories. Overall, the conversation highlights the complexity of black hole geometry and the evolving understanding in theoretical physics.