The galaxy presents as an edge-on spiral, characterized by a notably elongated morphology. The central bulge region exhibits a concentrated luminosity, transitioning into a fainter disk component. The bulge appears relatively smooth and rounded. The disk displays a higher degree of patchiness. Indications of minor internal disturbance within the disk cannot be ruled out, but there is no evidence of ongoing merger activity. A notable absence of distinct spiral arm structures is observed, with only subtle color variations.