The galaxy appears as a relatively smooth, elliptical-like structure with a slightly elongated morphology. It exhibits a concentrated central bulge, fading gradually into its outer regions. There is little evidence of spiral arms or distinct features typically associated with disk galaxies. The galaxy's color profile seems to be generally redder, suggestive of an older stellar population and a lower rate of on-going star formation. There are no visible signs of significant disturbances or major mergers impacting the galaxy's overall structure. The galaxy is a reasonably large galaxy, with an absolute magnitude indicating it's a fairly luminous object at its redshift.
