The galaxy appears as a flattened, elongated structure, viewed nearly edge-on. It exhibits a smooth, relatively featureless morphology. The central region shows a concentration of light with a slightly reddish hue, suggestive of an older stellar population or dust obscuration. Moving outwards from the center, the galaxy transitions to a bluer color. This suggests the presence of younger stars or ongoing star formation in the outer regions. No distinct spiral arms or bar structures are discernible in the image. There is no evidence of any significant tidal disturbances or ongoing mergers. The galaxy appears to be relatively isolated and undisturbed.
