This galaxy presents as a disturbed system, likely undergoing a merger event. Two distinct nuclei are visible, both exhibiting a relatively smooth, concentrated light profile. The larger of the two nuclei appears more luminous. A faint bridge of material seems to connect the two nuclei, though the resolution limits definitive confirmation. The overall color suggests a population of relatively young, hot stars and ongoing or recent star formation within the system. Tidal features, such as faint tails or plumes, may be present, however noise within the image makes it difficult to confirm these features.
