The galaxy appears as a relatively smooth, elliptical object with a noticeable central bulge. Its overall color is slightly reddish, suggesting an older stellar population with less ongoing star formation. The galaxy's shape is elongated, displaying an intermediate axis ratio, not quite circular but not extremely flattened either. There are no prominent spiral arms or distinct features visible, indicating a lack of significant dust lanes or regions of active star birth. No obvious signs of a major merger are present, although there might be a hint of minor asymmetry in the outer regions, possibly indicative of a past interaction or minor disturbance. The light distribution gradually decreases from the bright central bulge outward, exhibiting a smooth profile.
