The galaxy presents a largely smooth and elliptical morphology. The central region displays a concentrated brightness, shifting towards warmer yellow-orange hues, suggesting an older stellar population. Moving outward, the light becomes more diffuse with a slight greenish tint, though not distinctly indicative of active star formation on a large scale. The overall shape is somewhat elongated but is not highly deformed, indicating no major recent merger events, though a minor disturbance might be present. Its structure implies a significant spheroidal component dominates the galaxy. The galaxy's apparent size is relatively compact.
