The galaxy appears as a dual-component system, possibly undergoing a merger or interaction. One component presents as a relatively smooth, roundish, elliptical shape with a concentrated core and a redder color, indicating an older stellar population. The second component is more compact, exhibiting a bluer color, suggesting the presence of ongoing star formation. There may be some tidal distortion between these two components, indicating a possible interaction between them. The overall morphology suggests a system that is relatively settled, without major disturbances.
