This galaxy appears to be an elliptical galaxy at a moderate redshift. Its morphology suggests a system with a relatively smooth light distribution. The galaxy's color gradient indicates a redder core, likely populated by older stellar populations, with a bluer, more diffuse halo. The absence of any visible spiral arms or a prominent disk suggests that the galaxy is dominated by random stellar orbits and has likely undergone significant merging and relaxation in its history. While faint, a slight asymmetry in the outer regions hints at a possible minor interaction or past merger event, though the galaxy appears largely undisturbed at present. The measured size is compact and consistent with a relatively massive galaxy.
