The galaxy presents as a relatively smooth, elliptical-like structure. Its color profile suggests an older stellar population, with a dominant yellow-orange hue concentrated towards the center. The galaxy appears largely undisturbed, showing no strong evidence of ongoing mergers or tidal interactions. The light distribution is fairly even, with a slightly brighter core region. There is a subtle gradient in color, shifting toward redder tones in the central area and becoming slightly bluer in the outer regions, suggesting a possible difference in stellar age or composition between the core and the extended halo. Overall, the galaxy seems to be a relatively evolved system.