The galaxy exhibits a complex morphology, appearing as a system possibly undergoing interaction or a merger. A significant portion of the light is concentrated in a central region. The overall shape is neither perfectly elliptical nor a well-defined spiral, with indications of irregularity. Patches of blue suggest regions of recent or ongoing star formation, while redder components might represent older stellar populations or dust obscuration. There is evidence of tidal features or disturbances, suggesting gravitational interactions. The galaxy does not present a disk-like structure, although there could be some light extending from the center that might be an obscured disk. Overall, it appears to be a mid-sized galaxy.
