The galaxy exhibits a disturbed morphology, potentially indicative of a merger event. There appears to be a primary, centrally located, somewhat amorphous core. Emanating from this central region is a faint, elongated structure or tail, extending upwards in the image. The color is predominantly bluish, suggesting the presence of relatively young, hot stars. Some components of the galaxy appear more diffuse, while other regions seem to condense. The image shows evidence of tidal distortions, giving way to ongoing gravitational interactions. It is not a grand design spiral but a collection of interacting elements.
