The galaxy appears to be an elliptical galaxy. It exhibits a smooth, diffuse light profile with a concentrated central bulge. The overall shape is largely rounded. There is little to no evidence of spiral arms or distinct disk-like structures. There does not appear to be any major disturbances or tidal tails indicating an ongoing or recent merger event, although there is a very slight amount of disturbed dust. The galaxy's color indices suggest a relatively evolved stellar population, possibly with a significant presence of older, redder stars.
