The galaxy presents a somewhat amorphous appearance, lacking a clearly defined spiral or elliptical structure. The light distribution suggests a central concentration that is slightly diffuse. There is a hint of a disk-like structure, as the galaxy appears wider than it is thick, however, the galaxy is quite disturbed. Faint extensions are possibly detectable which could be the result of a minor merging event. This galaxy does not resemble an archetypal elliptical nor spiral galaxy. There may be an active galactic nucleus, but it cannot be confirmed from this image alone. Further spectroscopic data would be beneficial.
