Dwarf elliptical galaxies do exist near the Milky Way galaxy. These dwarf galaxies are small, faint, and lack the spiral arms and prominent structure seen in larger galaxies like the Milky Way. They are classified as dwarf ellipticals based on their shape and low surface brightness.
The Milky Way has several dwarf elliptical galaxies in its vicinity, which are often referred to as satellite galaxies or companions. The two most notable dwarf elliptical companions of the Milky Way are the Large Magellanic Cloud (LMC) and the Small Magellanic Cloud (SMC). These two galaxies are located relatively close to the Milky Way and are visible from the southern hemisphere.
The LMC and SMC are not only dwarf elliptical galaxies but are also irregular in shape. They are gravitationally bound to the Milky Way and are part of the Local Group, a small galaxy group that includes the Milky Way, Andromeda galaxy (M31), and several other smaller galaxies. The LMC and SMC are among the largest and brightest satellite galaxies in proximity to the Milky Way.
In addition to the LMC and SMC, there are several other dwarf elliptical galaxies orbiting the Milky Way. Some examples include the Sculptor Dwarf, Fornax Dwarf, Draco Dwarf, and Ursa Minor Dwarf galaxies. These dwarf galaxies are relatively small in size and often have a spheroidal shape, lacking the prominent spiral arms seen in larger galaxies.
Studying these dwarf elliptical galaxies near the Milky Way provides valuable insights into galaxy formation, evolution, and the dynamics of the local universe.