The galaxy presents as a moderately luminous object with a notable central concentration of light. The overall morphology is generally smooth and elliptical, exhibiting a high degree of radial symmetry. There is a slight elongation. Faint color variations suggest differential stellar populations within the galaxy. A smaller, fainter galaxy is in close proximity, and may be interacting with the primary galaxy. No prominent dust lanes or spiral arm structures are discernible in the image.
