The galaxy presents as a complex, multi-component system with a primary, brighter component and several fainter, possibly interacting, satellite structures. The primary component exhibits a smooth, somewhat elliptical morphology. Coloration suggests the presence of both older stellar populations, indicated by yellowish hues, and regions of ongoing star formation, evidenced by the presence of bluer patches. The system is likely undergoing some level of gravitational interaction or merger activity. A possible tidal stream is present, suggesting a recent or ongoing interaction with another galactic object. The galaxy appears relatively compact in size, but its absolute magnitude suggests it is a luminous galaxy. Based on morphology, the light emitted from the galaxy indicates that it is neither a perfect elliptical or spiral type galaxy. Its estimated mass falls in the range of a typical galaxy. There is evidence for possible recent starburst activity.
