The galaxy appears to be a relatively smooth, elliptical system. The light distribution suggests a centrally concentrated morphology with a significant spheroidal component. Its color is overall quite uniform, presenting as a yellow-ish hue, which is characteristic of older stellar populations and reduced ongoing star formation. There is no prominent evidence of spiral arms, dust lanes, or active star-forming regions visible. The object displays a high degree of circularity. There does not appear to be any significant tidal disruption or evidence of a recent major merger event. It is consistent with a relaxed system having undergone significant morphological transformation processes.
