This galaxy exhibits a complex morphology, appearing to be in a state of advanced interaction or merging. The primary body of the galaxy presents an irregular shape, with a dominant central region displaying a yellowish hue, indicating a population of older stars. Emanating from this core are faint, diffuse extensions suggesting tidal features or disrupted spiral arms. Patches of bluer light are interspersed throughout, possibly indicating regions of ongoing star formation triggered by the interaction. A secondary, smaller concentration of light is visible, suggesting another galactic component involved in the merger. The overall structure is not well-defined, indicating a significant level of gravitational disturbance.
