The galaxy presents as a relatively smooth, centrally concentrated object. Its morphology appears to be generally elliptical, exhibiting a moderate degree of roundness, though some elongation is present. The galaxy is a yellow-orange hue, which may suggest an older stellar population with relatively low recent star formation. No distinct spiral arms or other prominent features are discernible from this image. There is no visible evidence of significant tidal disturbances or ongoing mergers, though minor asymmetries cannot be ruled out. The galaxy's structure indicates it has likely undergone substantial evolution, potentially through past mergers or interactions.
