The galaxy presents as a spiral type, exhibiting a clear disc structure. Prominent spiral arms are visible, tracing a fairly well-defined pattern outward from the central region. The winding of these arms appears to be intermediate, neither tightly wound nor completely loose. A notable feature is the presence of a bar-like structure that crosses through the galactic nucleus. The nucleus appears somewhat obscured. The bulge component is observable but does not dominate the overall appearance; it is moderate in size. The disk appears relatively undisturbed without significant signs of major mergers or tidal disruptions. 
