The galaxy appears to be a merging system or a galaxy experiencing significant tidal disruption. The central region presents a concentrated, luminous core, emitting light in the yellow-red range. The distribution of light suggests an old stellar population. The outer regions exhibit a disturbed morphology, showing signs of interaction or recent merger activity. Faint extensions and asymmetric structures are visible, indicating tidal tails or disrupted arms. These features have a slightly bluer tint compared to the core, possibly indicating some recent star formation triggered by the interaction. There is no clear spiral or elliptical structure. Overall, this appears to be an active system undergoing significant morphological transformation.
