This galaxy appears to be an elliptical galaxy with a smooth light distribution and an elongated shape. The core of the galaxy is bright and concentrated, with the light gradually fading towards the outer edges. The color is generally redder, potentially indicative of an older stellar population with minimal ongoing star formation. There is a slight hint of a disturbance on the right side of the galaxy which could indicate a possible tidal tail or the remnants of a past merger, but further observation is needed to confirm this.
