The galaxy presents as a centrally concentrated object with a relatively smooth morphology. Its overall shape appears elliptical, displaying a high degree of circularity with minimal elongation. The core region exhibits a yellowish-white hue, suggestive of an older stellar population and a lack of significant ongoing star formation. The outer regions display a more diffuse, bluish color gradient, potentially indicative of some younger stars or residual star formation. There is no clear evidence of spiral arms or a well-defined disk structure. The galaxy does not appear to be strongly interacting or undergoing a major merger, although there may be a very slight asymmetry.
