The galaxy appears to be a relatively smooth, centrally concentrated system. It exhibits an elliptical morphology, appearing quite rounded in shape. There's no strong evidence of distinct spiral arms or a prominent disk structure. The central region is noticeably brighter, suggesting a concentrated nucleus or bulge component. The overall color appears to be in the green-blue range, which could indicate some ongoing, low-level star formation. No major disturbances or signs of an ongoing merger event are readily apparent. Faint, diffuse outer regions are observed, implying a gradual decline in stellar density with increasing radial distance from the center. 
