The galaxy appears to be an elliptical galaxy with a smooth, concentrated light profile. Its color index suggests a relatively old stellar population, with a lack of significant ongoing star formation. The galaxy exhibits a high degree of circularity with no apparent spiral arms or disk-like features. There is no evidence of any major or minor mergers. The morphology is consistent with an early-type galaxy located at cosmological distances, which can be expected to have a low star formation rate.
