The galaxy presents a largely smooth, elliptical morphology. The luminosity profile suggests a centrally concentrated bulge that fades outwards. The overall color is yellowish, indicating an older stellar population with lower rates of ongoing star formation. The lack of distinct spiral arm structures or significant dust lanes further supports its classification as an elliptical galaxy. The galaxy appears relatively isolated, showing no obvious signs of tidal distortions or nearby interacting companions, suggesting no recent major merger events. There may be a minor disturbance in the outskirts of the galaxy; further observations required.
