The galaxy presents as a spiral type, exhibiting a distinct disk structure. The arms are well-defined and numerous, primarily displaying a medium to loose winding pattern. A central bulge is present but appears relatively small to moderate in size compared to the overall galactic disk. The light distribution suggests ongoing star formation activity, particularly within the spiral arms. The overall color indicates a mix of stellar populations. There are no obvious signs of significant tidal distortions or major mergers.
