The galaxy appears to be an elliptical type, showing a generally smooth, centrally concentrated light distribution. It exhibits a slightly elongated shape that could be described as in between round and cigar shaped. A possible minor disturbance is visible as a faint, irregular extension, which may indicate an ongoing or past interaction with another galaxy. The color suggests the presence of evolved stellar populations, with a possible region of enhanced star formation indicated by a slightly bluer hue in one area. The galaxy is relatively bright, suggesting a high stellar mass. Evidence suggests it may be undergoing a merger, and potentially it is interacting with another galaxy.
