The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile appears predominantly yellow and orange, indicative of an older stellar population. There is some evidence of bluer colors in the outer edges of the galaxy, this might be due to younger stars. The galaxy appears slightly elongated in shape. It is plausible that the galaxy is undergoing a minor interaction with a smaller companion. The galaxy has an estimated stellar mass of approximately 10^10 solar masses. The star formation rate is modest but not negligible, suggesting ongoing but subdued stellar nurseries. This galaxy likely resides at a moderate cosmological distance and exhibits a relatively low specific star formation rate, consistent with galaxies of substantial mass and evolved stellar populations.
