The galaxy presents as a centrally concentrated, relatively smooth object. The morphology is largely elliptical, exhibiting a high degree of circularity, showing minimal deviation from a perfectly rounded shape. There is no apparent disk structure, and the galaxy appears to be largely featureless, with the suggestion of very minimal disturbed light. A color gradient is observed, with the core exhibiting a bluer hue and the outer regions appearing redder. This may indicate ongoing, though subdued, star formation within the nucleus with an older stellar population existing outwards. The overall lack of prominent features suggests a relaxed system.
