This galaxy presents a smooth, centrally concentrated morphology. The light distribution is very regular and its shape appears mostly round, with only a slight elongation. It has a yellowish color, suggestive of an older stellar population dominating the light output. There is no apparent spiral arm structure or significant dust lanes visible. There is no obvious evidence of a major ongoing merger or strong tidal disturbances, although there might be very minor asymmetries that suggest some past interaction or minor disturbance. Based on its observed color and morphology, it is likely a massive galaxy with a relatively low rate of star formation. 
