The observed galaxy presents a morphology consistent with a disturbed system, likely undergoing a merger or interaction. The central region exhibits a bright, compact core, possibly indicative of an active galactic nucleus or intense star formation. However, the core is noticeably asymmetric and elongated along the vertical axis, indicating a non-equilibrium state. Extending from the core are diffuse, irregular arms or tidal features characterized by bluish hue. These indicate the presence of populations of young, hot stars. There are also hints of tidal tails or extended plumes emanating from the main body. The presence of these features suggests a past or ongoing gravitational interaction with another galaxy. Overall, the galaxy exhibits a complex and irregular morphology, suggesting ongoing dynamical processes are in play.
