The galaxy exhibits a spiral morphology with a prominent central bulge. The bulge appears to be moderate in size, contributing significantly to the overall luminosity of the galaxy. Spiral arms are visible, extending outwards from the central region, although their definition is somewhat fuzzy. The arms seem loosely wound. Evidence suggests moderate star formation. There is no obvious major merger, though the structure does not appear entirely undisturbed. The galaxy exhibits characteristics indicating a disk, and the disk is seen face-on. The galaxy color indicates that it is actively forming stars, giving it a blue tint in the outer region, while the inner region is more yellow/white. There may be a weak bar feature in the center.
