The galaxy presents a generally smooth, elliptical morphology. A bright, concentrated central bulge dominates its structure. The light emitted is yellowish-white, implying an older stellar population within the bulge, possibly with lower levels of ongoing star formation. The outer regions of the galaxy fade gradually, forming an extended halo. There are no obvious spiral arm structures, bars, or signs of active galactic nuclei, although a high luminosity of the central region could be obscuring some of these features. The overall shape appears relatively round, with no major distortions or indications of a recent or ongoing merger event. Close inspection suggests subtle irregularities in the outer isophotes, warranting further investigation into the possibility of minor tidal interactions or past merger events. The size seems relatively compact, suggesting a moderately sized elliptical galaxy at the observed redshift.
