The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated, spheroidal shape with a high degree of roundness. There is little evidence of spiral arm structures or significant disk-like features. The galaxy appears to be relatively undisturbed, with no clear signs of major mergers or significant tidal distortions, but a possible minor disturbance can't be ruled out. The color profile shows a relatively redder central region that fades out. This suggests an older stellar population dominates the overall light output. The estimated size indicates that we are observing a large and reasonably massive galaxy. The absence of prominent features and the smoother appearance are consistent with a more evolved system, likely at a distance where finer details are blurred.
