The galaxy in the image appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge with a radial decrease in surface brightness. The core displays a yellowish hue, indicating a population of older stars. There is little evidence of spiral arms or significant dust lanes, suggesting a lack of active star formation. The galaxy is generally round in appearance, with a slight deviation towards a more elongated shape. No signs of major disturbances or mergers are visible, suggesting it is an isolated system currently in a quiescent state.
