This galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears elliptical, exhibiting a high degree of circularity. The central region displays a bright, yellowish-white hue, suggesting a population of older stars. Surrounding the core is a fainter, bluish halo. There is a possible indication of a very faint disk. The overall structure lacks prominent features such as spiral arms or strong dust lanes, further supporting an elliptical classification. There is no indication of any major ongoing merger activity, but subtle disturbances might be present.
