The galaxy exhibits a disturbed morphology, appearing to be undergoing an interaction or possible merger. The main body shows a bright, concentrated core region exhibiting a blue-white hue, indicative of potentially active star formation. A significant tidal tail emanates from one side of the main body, extending outwards. This tail shows a color gradient, transitioning from a bluish tint near the core to a yellower, less intense color further out. The shape of the tidal tail suggests a gravitational disruption. The overall structure of the galaxy does not present a clear spiral or elliptical morphology; the overall shape is distorted and irregular. There is evidence of faint tidal debris surrounding the main galaxy. The tidal features appear clumpy, possibly indicating regions of enhanced density or star formation triggered by the interaction.
