This galaxy appears to be an elliptical galaxy. It exhibits a generally smooth and rounded morphology, lacking any distinct spiral arms or significant disc-like features. The galaxy presents a concentrated central bulge region that fades into a more diffuse halo. Color gradients are subtle, though the central region tends toward yellower hues, suggesting an older stellar population relative to the outer regions which appear slightly bluer. The galaxy shows no obvious signs of major mergers or tidal disturbances, though subtle irregularities in its outer halo cannot be ruled out without deeper imaging. Overall, the galaxy seems relatively undisturbed, suggesting a stable and evolved system. The red shift of this galaxy indicates that it is relatively far away, with its light stretched to the red end of the spectrum as it moves away from us.