The galaxy appears as a centrally concentrated object with a relatively smooth overall morphology. The core exhibits a bright, yellowish-white hue, suggesting a dense population of older stars. Proceeding outward from the core, there is a gradual transition to a more diffuse and slightly bluer disk-like structure, yet still with a generally smooth appearance. There is some indication of minor distortions, although no strong evidence of spiral arms or a distinct bar structure. A faint, extended halo is visible, encompassing the main body of the galaxy. Based on its overall appearance, it seems like a possible elliptical galaxy, or perhaps a lenticular galaxy viewed at high inclination. There is a hint of minor disturbances in the outer regions, but no major merger events are apparent. The overall color profile indicates a mix of stellar populations, with an older core and a younger, bluer disk component.
