The galaxy presents a somewhat elliptical morphology. It exhibits a primarily smooth appearance with a noticeable central bulge, although a faint disk-like structure is potentially present. The galaxy appears relatively undisturbed, with no immediately obvious signs of major mergers or tidal features. The color distribution suggests an older stellar population, with a higher concentration of redder stars within the central bulge, gradually transitioning to slightly bluer hues in the outer regions, indicative of possible recent star formation at the periphery. Overall, the galaxy appears to be a relatively massive system, at a significant cosmological distance given the observed redshift.