The galaxy presents a generally elliptical morphology, with a bright, concentrated central bulge region exhibiting a yellowish hue, suggesting an older stellar population. The outer regions are more diffuse and possess a slightly bluer tint, possibly indicative of more recent star formation, although this is less pronounced. There is a subtle suggestion of a disk-like structure, but the galaxy is not viewed edge-on. No strong evidence of ongoing major mergers or significant tidal disturbances is apparent from visual inspection; however, subtle asymmetries might suggest minor gravitational interactions in the past. The overall structure appears relatively smooth, with no prominent spiral arms or distinct morphological features readily discernible. The galaxy is relatively luminous and massive. The object is located at a considerable cosmological distance, as indicated by its measured redshift.
