The object appears to be a relatively compact galaxy. Its morphology suggests a mostly smooth profile. The primary component exhibits a near-spherical shape, with a high degree of central concentration. Color gradients suggest some differential stellar populations, with bluer light concentrated in the central regions, transitioning to redder hues in the outer halo. There appears to be some possible minor disturbances or tidal features in the outer regions, indicating past interactions or mergers. Overall, the galaxy exhibits characteristics of an early-type system.