The galaxy appears to be a relatively smooth, elliptical galaxy. The galaxy exhibits a centrally concentrated light profile, diminishing outwards. The primary color of the galaxy is a yellow-red, suggestive of an older stellar population with lower rates of star formation. There are subtle color variations across the galaxy, but overall, it appears to have a well-mixed stellar population. There is little evidence of spiral arms or significant dust lanes, further supporting its classification as an elliptical galaxy. Based on the roundness of the profile, it is likely closer to an E0-E3 elliptical. There is no visible evidence of any major or minor mergers.
