The galaxy presents as a spiral type, exhibiting a significant disk component with well-defined spiral arms. The arms appear relatively tightly wound toward the center, and are somewhat clumpy. There is evidence for a weak bar structure, with enhanced emission along the center, suggesting increased activity. A substantial bulge is present, showing moderate emission that does not dominate the overall structure. The galaxy displays an inclination relative to the line of sight, with a degree of flattening observed. There's a clear color gradient, with bluer tints in the spiral arms that transitions to more red in the central bulge. The overall appearance suggests ongoing star formation. There are no obvious signs of tidal interactions or recent mergers.
