The galaxy appears as a lenticular or possibly an edge-on spiral galaxy. Its form is elongated with a high degree of ellipticity, suggesting a significant bulge component. The light distribution is smooth and concentrated towards the center, displaying a distinct central brightening. There is little to no visible structure, such as spiral arms or dust lanes. The galaxy exhibits a blueish hue and appears to have a moderate rate of star formation. There is no noticeable indication of recent major merger activity or significant tidal disturbance.
