The galaxy presents as a centrally concentrated, elliptical-like structure. The light profile appears smooth and diffuse, indicative of an older stellar population. The core is bright and gradually fades toward the outer regions of the galaxy. There is a slight elongation, with an approximate ratio of major to minor axis of 1.25:1, with a relatively high degree of axisymmetry. There is a possible slight distortion in the upper region of the image that may be a tidal feature, but it may also be an artifact of the image.
