The galaxy presents as a fairly smooth, elliptical-like structure with a concentrated central bulge. It appears to be relatively undisturbed, lacking significant tidal features or evidence of ongoing major mergers. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to a slightly redder halo. This color profile suggests an older stellar population dominating the galaxy's overall light output, with a subdued rate of current star formation activity. The galaxy's moderate redshift indicates it is at a significant cosmological distance. Its apparent size is small, implying a moderate physical size despite its considerable luminosity. Overall, the observed morphology is consistent with an evolved galaxy dominated by older stellar populations.
