The galaxy presents as a relatively smooth, rounded object with a concentrated central bulge or core. Its overall color profile is a blend of yellowish-white in the center, subtly transitioning to a bluish halo extending outwards. This suggests a stellar population that is older and redder in the core, surrounded by a younger, bluer population in the outer regions. There is a faint indication of a possible disk structure within the bluer outer regions, though distinct spiral arms are absent. The galaxy does not appear to be undergoing any major merging or tidal disruption events based on its overall smooth morphology. Its moderate redshift indicates it is at a considerable cosmological distance from our own galaxy.
