The galaxy presents as a singular, relatively smooth object. Its morphology appears elliptical, exhibiting a high degree of radial symmetry. The color profile is dominated by yellow and red wavelengths, suggestive of an older stellar population and a relatively low rate of current star formation. There is no obvious spiral structure or significant dust lane features visible. No tidal tails or other signs of major interactions are discernible, although some minor disturbances are possible based on the slight irregularities in the outer isophotes. The galaxy exhibits a compact appearance with no extended halo.
