The galaxy presents as a largely featureless elliptical system with a high degree of central concentration. The light profile appears smooth and symmetrical, suggesting a lack of significant ongoing merger activity or strong tidal interactions. There's a slight elongation, but it remains generally rounded. The central region exhibits a yellow-orange hue indicative of an older stellar population, which fades into a bluish halo at the edges. While some faint wisps may exist in the outer regions, they are not clearly defined and don't disrupt the overall smoothness. The galaxy seems to be relatively isolated.
