The galaxy exhibits an irregular morphology, appearing to be in a state of merging or strong interaction. There are two distinct nuclei, or bright central concentrations of light, suggesting that it is likely the result of two galaxies colliding. The primary colour is yellowish, indicative of an older stellar population. There are no clear signs of spiral arms or a defined disk structure. A small degree of tidal disturbance or minor irregular structure is present around the merging system, but they are faint and do not extend far from the core of the galaxy. Overall, the object appears to be a merging system of substantial mass.
