The galaxy presents as a relatively smooth, centrally concentrated object. Its color suggests the presence of an older stellar population. The morphology is predominantly elliptical, with the axial ratio suggesting a near-spherical shape, although slight deviations from perfect circularity are present. There is no obvious disk structure or spiral arm features. There are no major disturbances or mergers, although the light surrounding the galaxy suggests very minor disturbances. It appears to be relatively compact, with a small effective radius.
