This galaxy exhibits a disturbed morphology, suggesting it is undergoing or has recently undergone a merger event. The main body of the galaxy appears elongated, with a defined central bulge that shows a yellowish hue, potentially indicating an older stellar population. Extending outwards from the central region are irregular, diffuse structures that appear bluish, which may be indicative of ongoing star formation. There are also prominent tidal tails emanating from the main body, further supporting the hypothesis of a recent interaction. The galaxy is disk-dominated and a bit edge-on, with evidence of asymmetry in its structure. Overall, the galaxy appears to be in a state of transition, with significant morphological disturbances.
