The galaxy appears as a relatively compact, centrally concentrated object. Its morphology is predominantly smooth, displaying a nearly circular shape with no readily discernible spiral arms or bar-like structures. There's a subtle color gradient, with a yellowish-white core gradually transitioning to a dimmer, slightly reddish halo or outer region. No significant tidal disturbances or ongoing mergers are obvious from the image. The light distribution suggests that this galaxy could be an elliptical galaxy or a lenticular galaxy with a prominent bulge. Given its redshift, the galaxy is relatively distant, implying that the light we observe now was emitted when the universe was younger. This smooth structure indicates it is likely an older galaxy with a reduced rate of star formation.
