NGC 7507 is an elliptical galaxy located in the constellation Sculptor. It was discovered by the German-British astronomer William Herschel on October 30, 1783. The galaxy lies at an estimated distance of 80.1 million light-years (24.55 Mpc) from the Milky Way, and has an angular size of 2.0′ × 1.9′ in the near infrared. It is receding with a heliocentric radial velocity of 1,590 km/s. The morphological classification of NGC 7507 is E0, indicating an elliptical galaxy with an almost perfectly circular profile. This massive galaxy is fairly isolated, although it forms a pair with the barred spiral galaxy NGC 7513. The latter lies at a projected angular separation of 18′. Apart from a central dust lane, NGC 7507 displays neither shells nor tidal features. The stellar halo has two components, with the outer and inner halos counter-rotating. It is unusual galaxy in that it displays a negligible dark matter profile, showing a constant mass to light ratio. This apparent lack of a dark matter component is difficult to explain in an LCDM cosmology. The globular cluster population around NGC 7507 is very small, being only a tenth the size of other comparable ellipticals. It more closely resembles the globular population of a spiral galaxy.
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