The galaxy presents as a somewhat disturbed system with an intermediate redshift. It exhibits a mixed morphology, showing characteristics of both a smooth spheroid and a more disk-like structure. The light distribution is uneven, suggesting a complex internal structure, possibly the result of an interaction or merger event. There may be some ongoing star formation. The overall color profile indicates a mix of stellar populations, with both older and younger stars contributing to the observed light. There are some disturbances, or possibly faint tidal features, implying gravitational interactions with another galaxy nearby.
