The galaxy exhibits a complex morphology, appearing to be in the process of a significant merger. The central region displays a concentrated, yellowish core, indicative of an older stellar population. Extending outwards from this core are multiple distinct luminous components, suggesting ongoing tidal interactions and star formation activity. One of these components has a bluer hue, potentially indicating recent or ongoing star formation. The overall shape of the galaxy is highly irregular, lacking a clear spiral or elliptical structure, with a suggestion of significant disturbances in its morphology. The merging process appears to be in a relatively advanced stage, with significant overlap between the interacting components. Some regions exhibit diffuse, extended emission, possibly representing tidal debris or gas stripped from the progenitor galaxies.
