The galaxy presents a largely smooth morphology, exhibiting a near-circular shape.  The dominant light appears to originate from an elliptical distribution.  A color gradient is observed, with a redder core gradually transitioning to a greenish-yellow outer region. No spiral arm structure or obvious dust lanes are discernible in this image.  The galaxy appears relatively undisturbed, with no major signs of ongoing or recent merger activity.  Minor disturbances cannot be ruled out due to the resolution.
