This galaxy appears to be an interacting system undergoing a merger. Its morphology suggests a late-stage interaction. The primary component exhibits a somewhat elongated shape, significantly deviating from a perfect ellipse. The central region appears more concentrated and exhibits a yellowish hue, suggestive of an older stellar population. A fainter tidal tail extends outwards from the primary body, with some knotty structure within it. This tail is bluer in color, possibly due to ongoing or recent star formation induced by the interaction. The overall structure suggests a system that has experienced considerable gravitational disruption, evidenced by the irregular shape and the presence of extended tidal features. There is a possible second object or structure to the side.
