The galaxy presents an overall elliptical morphology, appearing relatively smooth with a high degree of central concentration. The light profile seems to lack prominent spiral arm structures or distinct features. The color gradient suggests a stellar population that is likely dominated by older stars, contributing to its redder appearance. There is a slight asymmetry, with a possible tidal tail or minor disturbance visible on one side, indicating a potential past or ongoing interaction with another galaxy or intergalactic material. The overall appearance suggests a relatively evolved galaxy, possibly undergoing or having undergone a period of star formation quenching.
