The galaxy appears as a centrally concentrated, moderately luminous object. The overall color is yellowish-white, suggesting an older stellar population with few young, massive stars. There appears to be no discernible disk structure or spiral arms; the light distribution is relatively smooth and even. Its shape is somewhat irregular but appears to be trending towards an elliptical or lenticular morphology. There is no evidence of a recent major merger or tidal interactions and no apparent active galactic nucleus. It is likely a massive galaxy with an estimated mass between 10^10 and 10^11 solar masses. The galaxy is observed to be actively forming stars at a low rate.
