The galaxy presents an overall disk-like morphology, though it appears relatively smooth in structure. A bright, concentrated central bulge is prominent, displaying a somewhat circular profile. The bulge transitions into a broader, more diffuse disk component. The disk is oriented roughly edge-on from our perspective. There are no obvious spiral arm structures or large-scale disturbances visible within the disk; although there may be some minor asymmetries in the outer regions. The galaxy exhibits a general blue hue, which is mostly concentrated around the central region, with a slight shift towards redder tones in the outer areas of the disk, suggesting a difference in stellar populations and age.
