The galaxy appears as a slightly elongated, lenticular or early-type spiral galaxy. It exhibits a smooth, concentrated light profile, with a brighter central bulge dominating the structure. Some faint traces of a possible disk structure are present, although these are not sharply defined.

The color of the galaxy is predominantly yellow, suggesting an older stellar population with minimal on-going star formation. The absence of strong blue colors indicative of young, hot stars suggests that it is either a passive galaxy or has a very low star formation rate. The morphology of the galaxy does not show any strong distortions or tidal features, suggesting that it has not undergone a major merger in recent history, although minor disturbances cannot be excluded. The object presents an intermediate roundness.

The overall appearance is consistent with a massive galaxy that has largely exhausted its gas supply and is passively evolving.
