The galaxy appears to be a relatively smooth, elliptical system. The central region exhibits a high concentration of light, suggesting a prominent galactic nucleus. The overall color is yellowish-red, indicating an older stellar population with minimal ongoing star formation. There is little evidence of spiral arms or a distinct disk structure. The galaxy appears fairly isolated, showing no signs of recent major mergers or significant tidal disturbances. The morphology suggests a system that has largely exhausted its gas supply, resulting in a quiescent state of star formation. The overall shape is close to round.
