The galaxy presents as a centrally concentrated, smooth object with a yellowish-orange hue. There is minimal evidence of spiral arm structures or distinct features like dust lanes. The overall shape approximates a spheroid, though it is not perfectly circular. The light distribution is concentrated towards the center, suggesting a dominant bulge component, with a gradual fading towards the outer edges. There are no clear indications of tidal tails or strong interactions that would denote an ongoing major merger event, but there appears to be some minor disturbance. The color suggests an older stellar population.
