The galaxy presents a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge characterized by a yellowish hue, suggesting a population of older stars. The overall shape appears more "in between" round and elliptical rather than perfectly spherical or highly elongated. There is very little indication of disk-like structures or spiral arms. No obvious signs of ongoing major mergers or significant tidal disturbances are apparent within the galaxy's structure. The overall color profile is dominated by redder wavelengths, indicative of a more quiescent stellar population and potentially lower star formation rates, particularly when considering the relatively high redshift. There is a slight increase in intensity in the very center of the galaxy.
