The galaxy presents as a centrally concentrated, elliptical structure. The core region exhibits a bright, yellowish-orange hue, suggestive of an older stellar population. A gradual decline in surface brightness is observed moving outwards from the central core. The outer regions display a more diffuse and indistinct morphology with a bluer color. The overall shape of the galaxy appears somewhat elongated. There is no evidence of strong spiral arm structures or significant dust lanes. Subtle indications of minor disturbances may be present, possibly indicative of a past or ongoing minor interaction or merger event.
