Through telescopes, the appearance of galaxies can vary significantly depending on factors such as their distance, orientation, and the wavelength of light observed. Spiral galaxies may reveal intricate spiral arms, while elliptical galaxies appear as smooth, featureless ovals. Additionally, telescopes sensitive to different wavelengths can unveil hidden structures, such as dust lanes and star-forming regions, providing insights into a galaxy’s composition and dynamics.
Come for the Scenery, Stay for the Stars