The galaxy presents as a relatively smooth, elliptical structure. The core exhibits a high degree of luminosity, decreasing radially outwards. There appears to be minimal discernible spiral arm structure or dust lane obscuration in the primary body of the galaxy. The light distribution suggests a spheroidal morphology, and it is primarily uniform in color. There is a secondary, much smaller object nearby that could possibly be tidally interacting, or simply in the line of sight. The primary galaxy appears generally undisturbed with no major mergers present. Its profile indicates that its shape is generally round. 
