The galaxy presents as a spiral type, displaying a prominent disk structure. Spiral arms are readily discernible, appearing to be somewhat tightly wound around the central bulge. The bulge itself seems moderately sized relative to the overall disk. A possible bar feature is visible bisecting the bulge, although it is not strongly defined. The disk shows evidence of substructure and star formation regions, indicated by variations in color and brightness along the spiral arms. No obvious signs of major merger events or tidal disturbances are immediately apparent, although minor irregularities in the disk's morphology cannot be ruled out. The galaxy is not observed edge-on, offering a clear view of its spiral structure.
