The galaxy presents as a relatively smooth, elliptical object. It appears to be largely spheroidal in shape, with minimal visible disk structure. The light is concentrated in the central region, indicating a prominent galactic bulge. There is a color gradient, trending from a yellowish core to a slightly redder hue in the outer regions, which may indicate an older stellar population in the core. There is no distinct spiral arm structure, bar, or dust lane visible within the galaxy. There may be some signs of minor disturbance.
