The object appears to be a galaxy undergoing a significant interaction or merger. The morphology is highly disturbed, with an irregular shape and no clear spiral arms or elliptical structure visible. A bright central region is discernible, possibly indicating an active galactic nucleus or a region of intense star formation. Faint extensions or tidal tails are present, suggesting gravitational interactions with another galaxy. The galaxy exhibits a bluish hue, which suggests the presence of young, hot stars. Dust lanes are not clearly visible, indicating a relatively low dust content or obscuration due to the merger activity. The overall appearance is indicative of a system in a state of dynamic evolution.
