The galaxy presents as a single, luminous object with a centrally concentrated light profile. The shape appears roughly elliptical, with a high degree of circularity. The galaxy displays a relatively smooth texture, with no discernible spiral arms or significant dust lanes evident at this resolution. There is a color gradient from the center outwards; the core region appears yellowish-white transitioning to a reddish-orange hue in the outer regions. This color suggests an older stellar population. There is no significant evidence of recent major mergers or tidal disturbances. The galaxy's appearance is consistent with an early-type galaxy, specifically an elliptical or lenticular type. The light distribution suggests that the system may be composed of evolved stellar populations.
