The galaxy exhibits a morphology suggestive of a merger event. Two distinct, somewhat diffuse central luminous regions are observed, connected by a less luminous, more diffuse bridge of material. The overall shape is irregular, departing significantly from elliptical or spiral forms. There are hints of tidal tails or distorted arm-like structures extending outward from the main body, though the image resolution limits definitive confirmation. The galaxy presents a color profile that is primarily yellowish, with a hint of bluer regions surrounding the connecting bridge, possibly indicating regions of increased star formation. The morphology suggests a system undergoing significant gravitational interaction, likely to result in a single, more relaxed galaxy in the distant future.
