The galaxy presents as a centrally concentrated, yellowish elliptical. It displays a smooth, relatively featureless morphology, with no prominent spiral arms or distinct dust lanes visible. The light distribution suggests a centrally dominant bulge component. The color gradient indicates the presence of a older stellar population dominating its light. It appears to be largely undisturbed, with no clear signs of ongoing major merger activity. The shape shows a intermediate axis ratio, appearing neither perfectly spherical nor highly elongated. There may be subtle hints of a disk component, but these are difficult to discern at this resolution. There are no nearby merging companions that can be seen.