The galaxy appears to be an elliptical galaxy. It presents a smooth, symmetrical morphology with a high degree of central concentration. There is no discernible disk component, spiral arm structure, or dust lane visible. The galaxy exhibits a color gradient, transitioning from a yellowish core to a slightly redder halo. The ellipticity is moderate, leaning towards a round shape. There is no indication of ongoing major merger activity or significant tidal disturbances. Subtle asymmetrical features suggest possible minor gravitational interactions or past minor mergers. Overall, the galaxy appears to be a relatively evolved system with little current star formation.
