The galaxy presents as a system exhibiting possible merger activity. There is an irregular shape to the overall galactic structure, indicating a deviation from a typical elliptical or spiral morphology. Two main concentrations of light are visible, one larger and more diffuse, the other smaller and more concentrated. These could represent the cores of the merging galaxies. The color gradient across the galaxy is non-uniform, with a shift towards redder hues in some areas, particularly within the more diffuse component, possibly indicating an older stellar population or dust obscuration. Evidence of bluer tones in other regions may denote ongoing star formation. Overall, the galaxy appears relatively smooth, with little indication of well-defined spiral arms or a prominent central bulge. There may be some minor disturbances or tidal features present in the galaxy.
