The galaxy presents as a relatively smooth, elliptical-like structure. Its overall shape is moderately round, with a slight deviation towards an elongated form. There is a hint of internal structure but it is not readily defined, although a faint disk-like feature is suspected, with no obvious spiral arms. There is no evidence of a major merger event, although minor gravitational disturbance or interaction cannot be ruled out, as evidenced by some asymmetry in the overall structure. The galaxy displays a central bulge, with decreasing luminosity outwards. The object is relatively compact, and has an apparent size indicating that it is likely moderately distant. Color gradients suggest older stellar populations are dominant within the galaxy.
