The galaxy presents as a relatively smooth, elliptical-like structure. It has a bright, concentrated central region that fades gradually outward. The morphology appears predominantly spheroidal, with a high degree of central concentration. It is more rounded than elongated. There is a faint, diffuse halo surrounding the core that has some blueish color. There is no obvious spiral arm structure present. A slight asymmetry may be present in the outer halo but it is difficult to determine due to the resolution and faintness. There is no major ongoing merging activity, although there may be a minor interaction or disturbance due to the asymmetry. Based on its color, which is yellowish in the central regions, it appears the stellar population is composed of older stars. The observed size suggests it is not particularly small, but not exceptionally large either.
