The galaxy presents as a fairly smooth, elliptical object, exhibiting a concentrated central bulge. The color profile is primarily yellowish-orange, suggestive of an older stellar population with diminished star formation activity. The galaxy appears relatively undisturbed, with no obvious signs of tidal interactions or major mergers, though a minor asymmetry cannot be entirely ruled out. The object is moderately extended, with a relatively high degree of roundness in its overall shape. A slight elongation is visible, hinting at a possible deviation from a perfect spheroid. There is also evidence of some internal structure, although it is subdued and not prominently defined, potentially due to its high redshift.
