The galaxy presents as a spiral galaxy. The galactic disc is clearly visible, exhibiting well-defined spiral arms. The arms appear relatively tightly wound around a central bulge. There is a distinct and compact yellow bulge. The color suggests the presence of an older stellar population within the bulge. The spiral arms themselves show hints of clumpy structure, potentially indicating regions of active star formation. The galaxy appears relatively undisturbed, with no obvious signs of major merger events or significant tidal distortions. There is an overall smooth structure, with a slight asymmetry.
