The galaxy presents a disk-like morphology, viewed at a moderately high inclination. There is evidence of a central bulge. The disk is relatively smooth. The light distribution is not uniform, with a clear concentration toward the center and a slight fading toward the outer edges of the disk. There is some subtle patchiness within the disk, hinting at possible spiral arm structure or dust lane absorption, though not strongly defined. The overall color is slightly blue, suggestive of ongoing star formation.
