The galaxy presents a generally smooth, elliptical morphology. The primary light distribution is centrally concentrated, exhibiting a high degree of radial symmetry. There is a subtle color gradient visible, with the core region appearing slightly more yellow and the outer regions exhibiting a bluer tint. No distinct spiral arm structures or prominent dust lanes are discernible in the image. Minor irregularities might be present, but are difficult to see due to the image resolution. The galaxy appears relatively undisturbed, showing no significant signs of ongoing major merger activity, however some minor disturbance may be present.
