The object presents as a galaxy with an elongated, irregular morphology. The light distribution suggests a central concentration with diffuse emission extending outward, forming a tail-like feature. The main body exhibits a color gradient, with a bluer hue towards one end and a redder hue towards the opposite end, potentially indicating differing stellar populations or dust obscuration. There is evidence of disturbances in the structure, possibly the result of tidal interactions or ongoing mergers. The relative lack of distinct spiral arms suggests a system that is either elliptical or a disturbed spiral, and based on its shape, it looks like a merger is occurring.
