The galaxy presents a smooth, elliptical morphology, with a concentrated central bulge and a gradual decrease in luminosity towards the outer regions. The color is generally yellow, indicating an older stellar population with less active star formation. There is a subtle asymmetry in the outer halo region, with a slight extension in the upper part of the image relative to the lower region. There are no readily identifiable spiral arms or distinct features of active star formation, such as HII regions or blue supergiant stars. The overall appearance suggests a galaxy that is relatively evolved, having undergone the majority of its star formation in the past.
