The galaxy appears as a centrally concentrated object, exhibiting a generally elliptical morphology. The light distribution is relatively smooth. There is a lack of readily discernible spiral arms or significant dust lanes. A subtle color gradient may be present, with the central regions appearing slightly yellower and the outer regions perhaps exhibiting bluer tones. This galaxy does not exhibit clear signs of ongoing merger activity or major disturbances in its structure, although very slight asymmetry cannot be ruled out with this image.
