The galaxy presents a somewhat elliptical morphology, appearing largely smooth in its overall structure. It appears to consist of two luminous, connected spheroidal components that are most likely cores of two distinct galaxies. These cores are characterized by a concentration of light in the redder wavelengths, suggesting older stellar populations. 

A fainter, more diffuse greenish halo surrounds these two galaxies. There are no obvious features to strongly suggest active star formation, but faint light in the blue-green wavelengths may hint at lower levels of ongoing star formation. The morphology also exhibits no pronounced spiral arms or a well-defined disk structure. Overall, it is difficult to tell if these are indeed two separate galaxies or a single entity in the process of merging. There is an asymmetry to the faint light and shapes of both galaxies which is suggestive of gravitational interaction between the two.
