The galaxy presents as a disk-shaped morphology, with a notable bulge in the central region. It exhibits a relatively smooth appearance, suggestive of a later-type classification. There's a clear gradient in color, transitioning from a yellowish core to bluish hues in the outer disk. This color gradient likely indicates the presence of younger, hotter stars in the spiral arms and older, cooler stars in the central bulge. There are indications of spiral arm structure, but they are not sharply defined. The galaxy shows a moderate degree of inclination relative to our line of sight, providing a view of its disk-like structure.
