The galaxy presents a flattened, disk-like morphology. Its central region exhibits a high degree of luminosity, appearing nearly saturated. The intensity decreases notably towards the outer edges of the galaxy. There is some indication of possible distortion or tidal features, most notably a slight asymmetry. The object exhibits signs of low-level disturbance, although not as prominent as a major merger event. The disk shows very little apparent structure or clear spiral arms. The overall color is indicative of a mixed stellar population, showing light across the g, r, and z bands. The outer regions are very faint. 
