The galaxy appears as a centrally concentrated, relatively smooth object. Its overall shape is elliptical, leaning towards being round rather than elongated. There is a noticeable colour gradient, transitioning from a yellowish-white core to a faint bluish halo. The smooth profile suggests a lack of prominent spiral arms or significant dust lanes. Some slight visual distortions are visible on the periphery. There is no strong evidence of a major merger event. The apparent smoothness, colour and shape suggest that this is likely a passively evolving galaxy with a lower rate of star formation, a population of older stars, and a substantial mass.
