This galaxy exhibits a disk-like morphology, with an overall bluish hue, particularly noticeable in the outer regions. The central bulge appears to be a more concentrated, smooth structure, with a whiter-yellow color. The disk shows some evidence of spiral arm structure, though the arms are not sharply defined, suggesting they may be somewhat flocculent or tightly wound. There is a slight inclination to the disk, as it appears somewhat elongated. No distinct dust lanes are visible, although there are hints of patchy obscuration within the disk. The galaxy does not appear to be undergoing any major mergers, though there may be some evidence of minor tidal disturbances or asymmetries in the outer disk, perhaps indicative of a minor interaction. Overall, the galaxy presents as a relatively normal spiral with ongoing star formation activity evident in the bluer regions of the disk.
