The galaxy presents as a spiral type, exhibiting a disk structure with a central bulge. Two well-defined spiral arms are visible, tracing a path outwards from the central bulge. The arms appear moderately wound, neither tightly coiled nor loosely extended. A faint, almost imperceptible bar-like structure may be present in the galactic center. The bulge appears relatively small compared to the disk, though it is quite prominent and features a yellow hue. There are regions of blue scattered along the spiral arms. The overall morphology suggests ongoing star formation. The galaxy displays no strong signs of a recent major merger, although subtle disturbances or irregularities in the arm structure cannot be ruled out. The disk is nearly face-on with no signs of being edge-on.
