The galaxy appears as a flattened, disk-shaped structure viewed nearly edge-on. The central region exhibits a brighter, more concentrated luminosity, likely indicative of a galactic bulge. A faint, extended disk stretches outwards from the central bulge, exhibiting a smooth texture with slight irregularities. A bluish hue is observable throughout the galaxy which may suggest active star formation in the disk. The overall structure indicates this is likely a spiral or lenticular galaxy. There is no strong evidence of active merging, though subtle asymmetries hint at possible minor disturbances.
