The galaxy presents a complex morphology, appearing as a system undergoing significant interaction or potentially a merger event. The primary body appears somewhat amorphous. The light distribution suggests a complex interplay of stellar populations, likely representing different stages of star formation or remnants of progenitor galaxies. There is evidence of potential tidal features or disrupted arms extending from the main body, indicating gravitational interactions. The system displays a mix of colors, with both yellowish and bluish regions observed. The bluer regions could indicate areas of active star formation, while the yellower regions may represent older stellar populations. The overall shape is not well-defined, indicative of a system that has been disturbed.
