The galaxy presents an irregular morphology, showing signs of disturbance. The light distribution is not smooth; there are clumpy features throughout. The central region appears brighter and more concentrated, though without a distinct nucleus. Some of these clumps show a distinct blue tint, which could indicate areas of recent star formation activity. There is also an extended component that is less concentrated and fainter, but which might still be associated with the galaxy. The irregular shape suggests possible past interactions or ongoing merging events. Overall, the galaxy does not appear to be a well-defined elliptical or spiral structure, with clear signs of dynamical disturbances.
