The galaxy presents a distinct spiral structure, with prominent, loosely wound arms emanating from a central region. Two arms are clearly discernible. Within the spiral arms, star-forming regions are likely present, indicated by the blue hue, which suggests the presence of hot, young stars. The galaxy appears to have a bar-like structure that is moderately strong running across the central part of the galaxy. This bar structure may be influencing the organization of the spiral arms. The central bulge is visible but it appears relatively small and non-dominant, suggesting a less evolved or pseudo-bulge. The morphology is generally undisturbed, though there may be some minor irregularities in the disk, suggesting a possible past interaction or minor merger. The galaxy is viewed at an angle not quite edge on, with a slight inclination.
