The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. There is no apparent spiral arm structure or bar. The light profile appears symmetrical and rounded, showing a gradual decrease in intensity from the core to the outer regions. The core itself appears unresolved. There is a subtle color gradient, with a slightly bluer hue around the outer edges and a redder hue dominating the central bulge. This color distribution may suggest ongoing star formation in the outer regions, contrasted with an older stellar population in the core. No significant tidal features or signs of recent major merger events are visible. The overall appearance suggests a relatively undisturbed galaxy, potentially an elliptical galaxy or a lenticular galaxy with a dominant bulge component.
