The galaxy appears as a moderate-sized object with a somewhat irregular morphology. A dominant, centrally located, smooth bulge-like structure is evident, appearing mostly uniform in color. Fainter, diffuse disk-like features extend from the central region; however, they are not sharply defined. The galaxy appears to be in relative isolation. The color distribution suggests older stellar populations, primarily in the central bulge. There may be slight evidence of disturbance or interaction in the extended disk.
