The galaxy in the image appears to be a disturbed system, possibly undergoing a significant merger event. The main body of the galaxy exhibits a somewhat elongated morphology. It exhibits a bright, moderately compact core region.

A prominent tidal tail extends from the main body, suggesting strong gravitational interactions. The tail is bluish in color, indicating the presence of young stars. The overall structure seems irregular, with no clear spiral arms or elliptical features immediately apparent. There might be some ongoing star formation within the galaxy, given its moderate luminosity. The system's disturbed morphology suggests a relatively high rate of mergers and interactions.
