The galaxy exhibits a central bulge with a notable concentration of light, displaying a smooth, yellowish-orange hue. Emanating from this bulge is a disk component. It appears to have spiral arm structures that are somewhat flocculent and not sharply defined. There are hints of bluer regions within these arms, suggesting areas of more recent star formation. The overall color gradient suggests a mixed stellar population, with older stars concentrated towards the center and younger stars scattered throughout the disk. There's no obvious signs of major mergers or strong tidal disturbances, though some asymmetry within the disk is visible.
