The galaxy presents an overall disk-like morphology, observed at a nearly edge-on orientation. A central bulge region appears with a brighter, more concentrated luminosity. The disk shows a smooth appearance, and the arms may contain faint dust lanes on either side of the bulge. There are no indications of intense star formation regions or pronounced spiral structure. The system does not appear to be undergoing a major merger, but minor disturbances in the disk may be present. The galaxy displays a bluer hue in the central region, with colors becoming redder towards the outer regions.
