The galaxy appears to be an elliptical galaxy with a smooth, symmetrical morphology. The central region exhibits a high surface brightness, fading gradually towards the outer edges. The core appears slightly yellowish, potentially indicating an older stellar population. There is no distinct dust lane or spiral arm structure visible, reinforcing the classification as an elliptical galaxy. The galaxy exhibits a relatively round shape, with no obvious signs of tidal interactions or recent mergers. The color gradient suggests a lack of significant ongoing star formation within the galaxy.
