The galaxy presents a largely smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile, appearing brightest towards the core and gradually fading outwards. The shape appears mostly round but is slightly in between round and cigar shaped. There is a slight bluish tint in the light emitted and appears to be minimal dust absorption in the galaxy, suggesting relatively unobscured star formation, although at a moderate rate. There is no evidence of any major mergers occurring, although a minor disturbance cannot be ruled out. The estimated size of the galaxy is approximately 5 kpc in radius.
