The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, with a high degree of central light concentration that gradually decreases outwards. The color gradient suggests an older stellar population, with a relatively uniform bluish-white hue throughout the galaxy, indicating moderate levels of ongoing star formation. The galaxy lacks any prominent spiral arm structures or obvious signs of recent mergers or major disturbances. There's a slight elongation in its shape but overall it appears mostly round.
