At the heart of M104 lies a bright, spherical core dominated by a dense cluster of stars and interstellar gas. This central region, visible as a glowing white hub in images, harbors a supermassive black hole with a mass equivalent to billions of suns. Surrounding the core is a prominent dark band of dust and gas, forming the "brim" of the sombrero. This dust lane is densely packed with molecular clouds, where star formation occurs, and it obscures some of the core’s visible light, creating the galaxy’s distinct two-tone appearance. The combination of the bright core and the sweeping dust lane makes M104 one of the most recognizable galaxies in the night sky.

M104’s total mass is estimated to be around 80 billion times that of the Sun, a testament to its gravitational dominance within its galaxy group. The galaxy’s structure suggests it may have undergone past interactions with neighboring galaxies, which could have influenced the formation of its prominent dust lane and the concentration of mass in its core. Observations across various wavelengths, from radio to X-ray, reveal ongoing processes such as star birth in the dust lanes and energetic activity near the supermassive black hole. As a member of the Virgo Cluster of galaxies, M104 continues to be studied for insights into galaxy evolution, the role of black holes in shaping galactic structures, and the distribution of dark matter in spiral systems. Its striking appearance and scientific significance solidify its place as a landmark in the cosmic landscape.