The galaxy appears as a centrally concentrated, elliptical-like structure. It exhibits a relatively smooth light distribution with a high degree of central concentration. There's a gradual decrease in luminosity from the core outwards, lacking distinct features such as spiral arms or prominent dust lanes. The galaxy appears slightly elongated, and a hint of a disc is noted. No major ongoing merger events are apparent, though there is a minor irregularity. The color gradient suggests a redder population in the outer regions with bluer stars concentrated in the center.
