The galaxy presents a largely smooth morphology, with a dominant spheroidal component. The object exhibits a concentrated, round form with a fairly high degree of central light concentration and minimal disc-like structures. There is no evidence of ongoing major mergers or significant tidal disturbances affecting the galaxy’s structure. The overall color profile suggests a relatively evolved stellar population with a lower rate of ongoing star formation, dominated by older, redder stars. The estimated size indicates this is a relatively large galaxy at its redshift.
