This galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The light distribution is relatively uniform, exhibiting a gradual decrease in intensity from the core to the outer regions. There is a subtle color gradient with a yellowish center and a transition to slightly bluer hues in the outer regions. The galaxy appears to be close to elliptical in shape. There's no significant evidence of strong spiral arm structure or significant tidal disturbances that suggest a recent major merger event. Subtle irregularities or asymmetries exist, suggesting the possibility of minor interactions or internal dynamical processes, but the dominant impression is that of a fairly well-relaxed system. Its observed redshift places it at a significant cosmological distance, implying a substantial intrinsic luminosity and mass.
