The galaxy presents a generally smooth, centrally concentrated morphology. Its overall color is a muted yellowish-orange, suggesting an older stellar population. There is little evidence of distinct spiral arms or significant dust lanes. The object appears relatively round with no obvious tidal features or distortions indicating a recent major merger event. Subtle variations in the light distribution may indicate minor asymmetries or internal structures, but the dominant impression is that of a well-formed system with minimal ongoing star formation. It is estimated to be about 8.4 kpc in radius. The galaxy is a redshifted object implying that it is at a significant cosmological distance.
