In this context, the distribution of galaxies throughout the vast expanse of the universe is more likely to be uniform, on average, at least beyond the local supercluster structures (clusters of galaxies grouped together). Galaxies are found in clusters, superclusters, and filaments that stretch across vast distances, with vast voids in between. The density of galaxies may vary from region to region, but there is no evidence to suggest that there is a specific center of the universe where the density of galaxies is significantly higher than anywhere else.
The universe is immense and contains an estimated 2 trillion galaxies. As we observe the universe from Earth, we perceive the galaxies to be distributed relatively evenly in all directions, apart from local variations and concentrations. The cosmic microwave background radiation, which is the faint glow of light left over from the early universe, is remarkably uniform across the sky, further supporting the idea that the universe is isotropic and homogeneous on a large scale.
Therefore, it does not make sense, from a cosmological perspective, to assume that the center of the universe is inherently more crowded with galaxies compared to other regions of the universe. Rather, the distribution of galaxies is generally consistent with a uniform expansion and distribution across the vastness of the cosmos.
