The galaxy presents as a relatively smooth, elliptical-like structure. The light distribution appears centrally concentrated with a generally round morphology. The main body of the galaxy exhibits a color gradient, transitioning from a bluer core to a redder outer halo. There is little evidence of spiral arms or distinct features. There may be evidence of minor disturbances in the galaxy's structure, but nothing major. There also might be two central points instead of one, although not clear. The galaxy does not appear to be currently undergoing a major merger, nor do the features suggest a recent major merger event. The color suggests a moderate amount of past star formation, but it has slowed more recently.
