The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits a largely elliptical morphology with a high degree of radial symmetry. There is a lack of discernible spiral arms or prominent dust lanes. The light profile suggests a bulge-dominated structure with a gradual decrease in luminosity outward from the galactic nucleus. The overall color seems to be consistent with an older stellar population. Any signs of recent or ongoing major merger events are absent. There might be a very subtle asymmetry in the outer regions, possibly indicating a minor interaction or disturbance in its past. 
