The galaxy presents as a somewhat amorphous structure with an overall elliptical morphology. The central region exhibits a pronounced luminosity, appearing as a bright, concentrated core with a yellowish hue, suggestive of an older stellar population. Moving outward from the core, the light profile gradually decreases, with the outer regions displaying a slightly bluer tint. This suggests a possible mix of stellar populations, with ongoing, though perhaps modest, star formation in the galactic outskirts. There are some apparent asymmetries present, indicating possible gravitational interactions or recent minor mergers. The overall impression is that of a massive galaxy at an intermediate redshift, possibly in a transitional phase between a more actively star-forming system and a quiescent, redder galaxy.
