The galaxy presents as an elongated, disk-shaped structure, observed nearly edge-on. The central region exhibits a bright, concentrated luminosity, suggesting the presence of a significant bulge component. This bulge appears smooth and rounded. Fainter, diffuse material extends outwards from the central bulge, forming a flattened disk. The disk does not present any distinct spiral arm structures. There is no evidence of a major ongoing merger, though some minor asymmetry or disturbance cannot be ruled out at this resolution. The overall color is reddish, suggesting a population of older stars and a low rate of current star formation.
