The galaxy presents as a relatively smooth and elliptical structure. The central region exhibits a higher luminosity, gradually decreasing towards the outer edges. There is little evidence of spiral arms or a distinct disk. The color profile suggests a possible redder hue in the central bulge, with slightly bluer tones appearing towards the outer regions, which may indicate some low-level star formation activity. No obvious signs of any major mergers or significant tidal disturbances are apparent. The overall morphology is consistent with an early-type galaxy at an intermediate redshift, possibly undergoing some ongoing minor stellar formation.
