The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a mostly elliptical morphology with a high degree of roundness. The core region displays a bright, condensed appearance, possibly indicative of an active galactic nucleus or a high concentration of stars in the central bulge. There are subtle color variations, suggesting some spatial differences in stellar populations or dust content within the galaxy. Specifically, there may be hints of a disk-like component, although it is not strongly defined. There is no evidence of major mergers or significant tidal disturbances. Overall, the galaxy appears to be a massive system, likely an elliptical galaxy with a relatively low star formation rate.
