The galaxy presents as a flattened, disk-shaped structure viewed nearly edge-on. A prominent central bulge dominates the galaxy's core, exhibiting a smooth, yellowish hue that suggests an older stellar population. The disk component displays a complex structure with hints of dust lanes obscuring portions of the starlight. Faint blue-greenish emissions appear along the edges of the disk, possibly indicating regions of active star formation. The overall morphology suggests a relatively undisturbed system with no major signs of interaction or tidal disturbances.
