This galaxy appears to be an elliptical galaxy, exhibiting a smooth, spheroidal morphology. It displays a concentrated central bulge that is roughly spherical and appears to be quite large. The light emitted from the galaxy is mostly in the redder part of the visible spectrum, and the gradient is consistent from the center. Faint blue light is visible in the outer halo. This suggest the galaxy is largely composed of older stellar populations with relatively low star formation activity. There is no evidence of spiral arms or a prominent disk structure. There is no evidence of any major mergers occurring.
