The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and rounded morphology. It is characterized by a concentrated central bulge, which transitions smoothly to a diffuse halo. There is little evidence of spiral arms or significant dust lanes. The light is dominated by yellowish hues, suggesting an older stellar population, with redder light concentrated at the center. Given its redshift, the galaxy is relatively distant and its absolute magnitude is quite luminous. This suggests the galaxy is quite massive, likely in the range of billions to hundreds of billions of solar masses. Based on its morphology and color, the galaxy likely has a low star formation rate and a correspondingly low specific star formation rate. Interactions or mergers with other galaxies appear to be minimal, as there are no obvious tidal tails or morphological disturbances.
