The galaxy appears as a centrally concentrated, elliptical structure with a smooth, diffuse light distribution. The core is characterized by a bright, yellowish-white hue, suggesting an older stellar population dominating the central region. Moving outward from the core, the galaxy exhibits a gradual decrease in luminosity and a shift towards slightly redder colors in its outer regions, implying a potentially less active star formation rate than in the past. No distinct spiral arms or prominent dust lanes are apparent in this image, supporting the classification as an elliptical galaxy. The overall morphology indicates a system that is relatively relaxed and evolved. There may be minor disturbances or a hint of merging occurring, but the dominant characteristic is that of a smooth, spheroidal galaxy.
