This galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge, which appears more yellow in color suggesting an older stellar population. The outer regions appear to fade gradually into the background. Overall, the galaxy seems to be fairly isolated, without any signs of major disturbances or ongoing mergers. It has a moderate redshift, indicating a significant distance from our own. Based on its color and morphology, it appears to be a mature galaxy, likely with a lower star formation rate.
