The galaxy presents a somewhat smooth, yet evidently structured form. The central bulge appears moderate in size and exhibits a bright, concentrated luminosity, transitioning to a more diffuse and less luminous outer disk. Faint spiral arm structures are visible, although not prominently defined. There is suggestion of a weak bar structure bisecting the central region of the bulge. Overall, there does not appear to be any significant interaction or major disturbance affecting the galaxy's morphology.
