The galaxy presents as a relatively smooth, elliptical morphology with a slight elongation. The central region exhibits a concentrated, bright core, indicative of a likely bulge component. The color profile shows a predominantly red-yellow hue, transitioning to slightly bluer tones in the outer regions, suggesting a mix of older stellar populations in the core and possibly younger stars in the extended disk or halo. Evidences of significant ongoing star formation are not prominently observed in this imaging, thus suggesting the lack of spiral arms or large HII regions. There are no distinct signs of major disturbances or ongoing mergers; however, subtle asymmetries in the outer envelope could suggest a minor interaction in the past. Overall, this galaxy appears as a relatively evolved system with a moderate mass content, likely located at a considerable distance, indicated by its redshift.
