The galaxy presents as an edge-on spiral, characterized by a prominent, centrally located bulge that displays a smooth, rounded morphology. The disk appears relatively thin and extended, exhibiting a slight warp. There is little to no evidence of significant ongoing merger activity or major disturbances within the galactic structure, though a minor perturbation cannot be ruled out. The bulge appears yellow, consistent with an older stellar population. The galaxy shows some signs of star formation.
