The galaxy exhibits a disk morphology with prominent spiral arm structures. These arms are relatively tightly wound. The central bulge appears moderate in size, displaying a yellowish hue, suggestive of an older stellar population. The disk of the galaxy shows a distinct bluer color, indicating ongoing star formation within the spiral arms. There is no major disturbance, but some minor disturbance or merging cannot be ruled out. There appears to be some sort of bar, but it is difficult to ascertain the strength of the bar. The galaxy has no obvious edge-on presentation.