The galaxy presents a largely smooth morphology, appearing as a single, relatively unstructured luminous body. The light profile suggests a centrally concentrated system, with a gradual decrease in surface brightness outward from the core. Color gradients are subtle but appear to show a bluer hue in the outer regions compared to a more yellow-red central region. This could indicate a younger stellar population in the outer regions or dust obscuration in the center. The overall shape is generally elliptical or spheroidal, with a relatively high degree of roundness and no obvious spiral arm structures or a pronounced disk component. There are hints of minor asymmetries or disturbances in the outer regions, but no clear signs of a major merger or significant tidal interactions are evident.
