The galaxy presents as a relatively smooth and concentrated object. It exhibits an elliptical morphology, appearing elongated but not extremely so. There is a dominant central bulge, characterized by a yellow-orange hue, suggesting an older stellar population. The outer regions show a more diffuse and slightly bluer color, indicating the presence of some younger stars. The overall structure suggests a relaxed system, with no obvious signs of recent major mergers or significant tidal disturbances. Any star formation is likely occurring at a low rate. The galaxy appears fairly isolated, with no immediately apparent companion galaxies or strong interactions influencing its morphology.
