The galaxy presents as a single, moderately concentrated luminous object. It exhibits a generally smooth morphology, lacking distinct spiral arms or a prominent bar structure. The light distribution appears centrally concentrated with a radial falloff in intensity.  The galaxy's core presents a bright, yellow-white hue. There is a distinct, red-shifted object that appears to be interacting with the galaxy or is the result of merging activity. The system may be undergoing minor tidal distortions. It is plausible that we are observing a merger or strong interaction between a large galaxy and a smaller companion.
