The galaxy presents a largely smooth, elliptical morphology. It is characterized by a centrally concentrated brightness profile, with a gradual decrease in luminosity towards the outer regions. The galaxy exhibits a yellowish-orange hue, suggesting a stellar population dominated by older stars. The isophotes appear largely regular and concentric, with a slight deviation towards a more elliptical shape, but approaching round. There's a possibility of a very minor disturbance in the structure, but overall the galaxy seems relatively undisturbed. There is no clear evidence of spiral arms or active star formation regions within the galaxy. The light suggests that this is an evolved system with a low star formation rate.
