The galaxy presents as a relatively smooth, centrally concentrated object. It appears to be generally elliptical in shape, without any obvious spiral arm structure or significant disk component visible. The light distribution suggests a higher concentration of stars toward the center, fading gradually toward the outer edges. There is a slight colour gradient, shifting from a bluer hue in the central region towards redder tones in the outer regions, potentially indicating differences in stellar populations or dust distribution. No apparent tidal features, strong dust lanes, or signs of active galactic nuclei are immediately noticeable, and there appear to be no signs of a recent or ongoing merger, with the system appearing relatively relaxed.