The galaxy presents as a relatively smooth, elliptical structure. It displays a high degree of central concentration, with light intensity decreasing gradually from the core outwards. The isophotes appear largely regular, with a suggestion of slight ellipticity. There is no obvious evidence of spiral arms or a distinct disk component. The color is consistent with an older stellar population. Based on its morphology, this galaxy may be classified as an elliptical galaxy. There are no signs of any major disturbances.
