The galaxy presents an elliptical morphology. It exhibits a relatively smooth light distribution, with a concentrated central bulge that appears reddish in color. The outer regions of the galaxy transition to a less intense, greenish hue. Overall, there is little evidence of distinct spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, showing no indications of a major ongoing merger event, though a minor disturbance cannot be ruled out. Based on the red color, it is likely that this is a very massive galaxy with mostly old stars.
