The galaxy appears as a centrally concentrated, elliptical or spheroidal object. Its color profile suggests a predominantly older stellar population, appearing more yellow-orange than blue. There is a high degree of smoothness to its overall structure; distinct spiral arms or other defined features are not apparent. There is no strong indication of recent or ongoing major mergers, though the system is not perfectly isolated, possibly exhibiting minor disturbances. Its shape is consistent with a near-spherical morphology.