The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a bright, concentrated central bulge that dominates the overall luminosity. There is an apparent absence of well-defined spiral arms. The galaxy appears mostly rounded. The galaxy appears to be isolated, with no obvious signs of a major merger event. There is a small chance that a minor disturbance is taking place within the galaxy, but this is uncertain. The galaxy exhibits a slight color gradient, with the central bulge appearing more yellow-red, and the outer regions appearing more blue-green. The star formation rate in this galaxy appears to be low, indicating a more evolved stellar population. The galaxy has a high stellar mass.
