The galaxy presents as a smooth, elongated spheroid with a noticeable central bulge. It is likely an elliptical galaxy, or potentially a lenticular galaxy viewed at an angle. There is a slight color gradient, with the central bulge appearing more yellow-orange compared to the slightly bluer outer regions, which suggest differing stellar populations. The morphology suggests a system where star formation may have diminished, but is possibly still ongoing to some degree in its outer regions. It appears relatively undisturbed, with no significant tidal features or signs of a major ongoing merger. The galaxy possesses a substantial mass, with an estimated size of approximately 7 kpc across, indicating a relatively compact structure. Overall, this galaxy appears to be a well-formed, relatively quiescent system evolving toward a more passive state.
