The galaxy presents as a centrally concentrated, elliptical or lenticular system. The central bulge exhibits a smooth, relatively featureless morphology with a dominant yellowish hue, suggestive of an older stellar population and lower levels of recent star formation. There is a weak disk like structure with less yellow coloration and a hint of bluer light. The overall shape is slightly elongated, tending towards an oblate spheroid. A very minor disturbance may be present on one side, although nothing that suggests an active ongoing merger.
