This galaxy appears to be a relatively smooth, elongated system, likely an elliptical galaxy. The central region exhibits a concentration of light, appearing yellowish, which could indicate an older stellar population. The outer regions fade gradually, displaying a slightly bluer hue, possibly due to a younger stellar population. The galaxy appears undisturbed, without any obvious signs of recent major merger activity, although some minor disturbances cannot be ruled out based on this image alone. Overall, the object presents as a galaxy undergoing a moderate level of star formation within a relatively high mass system.
