The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The light profile suggests a bulge-dominated system with minimal discernible disk structure. A color gradient is present, transitioning from a yellowish hue at the core to a slightly redder color in the outer regions. This may indicate a more evolved stellar population in the central bulge compared to the outskirts. No distinct spiral arms or dust lanes are apparent, reinforcing the classification as an elliptical galaxy. The overall appearance indicates that the galaxy is relatively massive with a low rate of star formation. There is a slight asymmetry to the galaxy, possibly indicating that a small merger occurred. The galaxy appears to be relatively isolated. 
