The galaxy appears as a roughly elliptical structure with a bright, concentrated central core. The core is a high-intensity, unresolved source of light. Surrounding the core, there is a fainter, somewhat irregular halo or disk. The color distribution suggests a varying stellar population. The inner regions closer to the core exhibit a bluer hue, possibly indicating younger, hotter stars, while the outer regions have a slightly redder tint, suggesting an older population. There's a hint of structural irregularity, possibly indicating minor tidal disturbances or ongoing interactions with another galaxy. The overall form lacks well-defined spiral arms, indicating that this is likely an elliptical galaxy. The outer halo appears diffuse and ill-defined, fading gradually into the background sky. 
