The galaxy presents as a spiral type with a discernible disk structure. The disk exhibits a prominent bulge, seemingly of moderate size relative to the overall galactic structure. Observable are spiral arms, which appear somewhat tightly wound. There is a suggestion of bar structure across the central region of the galaxy. The galaxy does not present as an obvious edge-on disk. The colour profile suggests ongoing star formation, though the image quality makes further assessment difficult. There is no evidence to suggest ongoing major merger activity. The morphology shows signs of moderate bulge to disk ratio with arms that are visible as more luminous in color.