The galaxy presents as a diffuse elliptical, exhibiting a relatively smooth, featureless morphology. It has an overall slightly elongated shape. The color profile suggests a dominant population of older stars, with a yellowish-white hue concentrated towards the center. There are indications of some bluer regions, possibly indicating areas of more recent, albeit subdued, star formation. No distinct spiral arms or dust lanes are discernible. There is no significant signs of any major merger events. There may be a faint amount of active galactic nuclei activity present.
