The galaxy presents as a singular, relatively smooth structure. The light distribution suggests an elliptical morphology, with a high degree of central concentration and a generally round shape. It exhibits a central bulge that appears yellowish-orange, indicating an older stellar population, and suggesting minimal ongoing star formation within the core. Faint and diffuse light extends outward from the central region, gradually fading into the background. There is no readily apparent spiral arm structure, nor any signs of major tidal disturbances or active galactic nuclei activity in this image. The galaxy’s overall appearance suggests it is a massive elliptical galaxy that is relatively quiescent.
