The observed galaxy presents a complex morphology. Its apparent structure seems to display characteristics indicative of a potential ongoing merger event. There appears to be a disk like component near its center.

The central region is marked by a high concentration of relatively bright light, possibly indicating the presence of an active galactic nucleus or a very dense stellar population. The outer regions exhibit a more diffuse distribution of light, with indications of tidal tails or distorted arm structures. These faint extensions suggest gravitational interaction with another galaxy, lending further credence to the merger scenario.
