The galaxy presents as an elliptical or spheroidal system with a high degree of central concentration. Its morphology appears largely smooth, lacking prominent spiral arms or a well-defined disk. The light distribution is centrally concentrated, appearing round. There is a suggestion of a minor disturbance in the outer regions, however the galaxy's core is relatively undisturbed, with a high probability of no merger. The galaxy's color index suggests an aging stellar population. Overall, it is a luminous and relatively massive galaxy with a moderate redshift indicating significant distance. The star formation rate appears low.
