This galaxy appears to be an elliptical galaxy at a redshift of approximately 0.14, meaning it is relatively distant. It exhibits a smooth, concentrated morphology, with a high degree of central concentration and little evidence of spiral arm structure. The galaxy's light profile suggests it is primarily composed of an older stellar population, as indicated by its redder color indices, becoming less blue in each filter respectively. The galaxy shows an intermediate rounded shape that appears slightly elongated. No major disturbances or mergers are apparent in the visual structure.
