The galaxy appears to be a large, relatively smooth, elliptical galaxy. Its core is very bright and concentrated, with a yellowish hue, suggesting an older stellar population. There is a noticeable decrease in surface brightness from the core outwards, with a more diffuse halo of light extending beyond the central region. The galaxy is generally round, without any clear spiral arm structure or significant irregularities in its shape. There is little evidence of active star formation from this image alone. The overall morphology suggests a system that has undergone significant dynamical relaxation and quenching of star formation.
