The galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The core exhibits a bright, yellowish hue, potentially indicating an older stellar population. A subtle color gradient is apparent, transitioning from the yellowish core to a slightly bluer outer region, suggestive of some ongoing, though perhaps limited, star formation activity. The galaxy shows no evidence of significant spiral arm structure or major disturbances, indicating that it has not undergone a recent major merger. There is a minor degree of asymmetry, although this may be artefactual. The overall light distribution is relatively even, further supporting the smooth classification.