The observed galaxy presents a morphology indicative of an ongoing or recent merger event. The central region displays two bright, concentrated areas of light. These could represent the cores of the original galaxies prior to complete coalescence. One core appears more blue, suggesting a region of more recent or ongoing star formation, while the other has a more yellow/green hue, which could suggest an older stellar population or dust extinction.

A faint, diffuse bridge of light extends between the two cores. This could be stellar material stripped from the merging galaxies due to gravitational interaction. There is no clear disk structure visible, and the overall shape appears irregular rather than exhibiting well-defined spiral arms or a smooth elliptical profile. Faint tails or plumes can be seen extending outwards, further supporting the hypothesis of a merging system where tidal forces are disrupting the original galactic structures. The light appears relatively red indicating it is somewhat further away.
