The galaxy presents a largely smooth, elliptical morphology with a high degree of circularity. A bright, concentrated core is evident, characterized by a yellowish hue, suggesting an older stellar population. There is a subtle color gradient moving outward from the core to the edge, with the outer regions appearing slightly bluer, potentially indicating younger stars or lower metallicity. No distinct spiral arms or disk structure are visible in this image. There is no visually discernible evidence of significant tidal disturbances or ongoing major merger events. The overall light distribution appears relatively symmetric and undisturbed. Based on the observed color and morphology, the galaxy is likely an elliptical galaxy with a red shift suggesting a moderate distance from the observer. This galaxy appears to have a high mass. The estimated star formation rate is relatively low.