This galaxy exhibits a disturbed morphology, indicative of an ongoing or recent merger event. The overall structure is irregular, lacking a clear spiral or elliptical shape. Two distinct clumps of brighter luminosity are observed, possibly representing the cores of the merging galaxies or regions of intense star formation triggered by the interaction. A faint tidal tail extends outwards from the central region, suggestive of gravitational disruption. The galaxy shows a blueish hue, consistent with the presence of young, hot stars. There is a clear disk component, but it is being heavily disrupted by the merger event. The overall impression is one of dynamic interaction and significant morphological transformation.
