The object under examination presents a complex morphology, suggestive of a galaxy undergoing significant interaction or disturbance. The central region displays a relatively smooth appearance, indicating a possible bulge component. However, there are asymmetric features and faint extensions emanating from the core, particularly towards what appears to be the southern region of the object. These features could be tidal tails, indicative of gravitational interaction with another galaxy, or signs of internal disruptions. There is a secondary concentration of light located nearby, which suggests that this could be a close companion galaxy. Furthermore, there is a distorted arm-like feature that may also be caused by gravitational interaction. The central body appears somewhat rounded. The overall appearance of this galaxy complex is not that of a relaxed, elliptical system, but instead implies a dynamic state potentially induced by merging or ongoing tidal interactions. The differential color across the galaxy system suggests varying stellar populations.
