The galaxy appears to be an elliptical galaxy with a smooth, diffuse light profile, indicative of an older stellar population. There is some evidence of a slight disturbance in the galaxy's morphology, potentially indicating a past or ongoing merger event. The galaxy displays an elongated shape, with a noticeable tilt to its major axis. The color gradient shows a concentration of older, redder stars towards the central region, with slightly bluer regions further out, suggesting some ongoing star formation, possibly triggered by the merger. Overall, the galaxy exhibits characteristics of a mature system that has experienced gravitational interactions.
