NASA and ESA's Hubble Space Telescope has recently captured detailed images of multiple galaxies, providing new insights into their structures and characteristics. Among these is NGC 45, a low surface brightness galaxy located 22 million light-years away in the constellation Cetus. The telescope also imaged NGC 2146, a spiral galaxy where supernova explosions and stellar winds drive double star systems and hot gas away, with one of its dusty arms obscuring the galaxy’s center from Earth. Another notable observation includes NGC 3783, a bright barred spiral galaxy approximately 130 million light-years distant, part of a 47-member galaxy group. Hubble's Advanced Camera for Surveys revealed NGC 6684, a lenticular galaxy about 44 million light-years away in the constellation Pavo. Additional galaxies studied include NGC 247 in Cetus at 11 million light-years, NGC 3285B in Hydra at 137 million light-years, NGC 2442 in Volans at 50 million light-years with an asymmetrical shape, NGC 3596 in Leo at 90 million light-years, NGC 2283 at 45 million light-years highlighting star clusters and supernova activity, and NGC 1022, a barred spiral galaxy 65 million light-years away. The images combine multiple wavelengths, including visible light and X-rays from Chandra, to reveal features such as galactic nuclei, star clusters, gas clouds, and supernova remnants. Additionally, Hubble captured the supernova 1987A in the Large Magellanic Cloud, located 168,000 light-years away, notable for its glowing ring caused by the explosion’s shockwave interacting with expelled gas. These observations enhance understanding of galactic formation, structure, and the dynamic processes within various galaxy types across different constellations.