The galaxy exhibits a morphology indicative of an ongoing or recent merger event. The central region is a diffuse, luminous yellow, suggesting an older stellar population. Two distinct components are observed: a more compact, brighter yellow structure likely representing the core of one of the progenitor galaxies, and an extended, less luminous component. This extended component shows hints of blueish regions, possibly areas of active star formation stimulated by the merger. The overall shape is highly irregular, deviating significantly from a typical elliptical or spiral morphology, consistent with gravitational disturbances and tidal forces associated with the merger process. It is elongated and somewhat cigar shaped.
