The galaxy presents as a centrally concentrated, relatively smooth object. It exhibits a notable degree of sphericity in its overall shape. There is no apparent disk structure or spiral arm morphology discernible. The light distribution appears to be fairly even, with a strong central bulge. A subtle color gradient is observed, transitioning from bluer hues near the center to slightly redder tones in the outer regions. The galaxy does not show obvious signs of major disturbances or ongoing mergers, maintaining a largely undisturbed form. It likely has a mass of around 10^10 solar masses. Star formation may be occurring but is at a slow rate.
