The galaxy presents a disk-like structure, with a clear central bulge. Spiral arms are visible but are somewhat faint and tightly wound, suggesting a relatively evolved spiral galaxy. The galaxy appears to be barred, with the bar structure oriented roughly horizontally across the major axis. There is a moderate central bulge relative to the size of the disk. The color gradient from the center outwards indicates ongoing star formation, with bluer hues in the arms suggesting younger stellar populations, and a yellower hue toward the central bulge. There is no obvious sign of any major merger, but there might be minor disturbances. The galaxy appears relatively isolated.