The galaxy presents a smooth, elliptical morphology with a moderate axis ratio, appearing more in-between round and elongated rather than perfectly circular. The light distribution suggests a relatively uniform stellar population, with a dominant, older stellar population as indicated by the redder color. There are no apparent spiral arm structures or significant dust lanes visible, consistent with an early-type classification. Indications of ongoing or recent major merger activity are absent, though subtle disturbances cannot be ruled out. The galaxy's estimated size is relatively compact, but the absolute magnitude suggests it is a fairly luminous object. The galaxy's estimated star formation rate is quite low, and would be considered a very quiescent object.
