The galaxy presents with a disturbed morphology, indicative of ongoing or recent interaction. The main body of the galaxy appears elongated and irregular, lacking a clear spiral or elliptical structure. There is a distinct blueish hue, suggesting the presence of young, hot stars and active star formation. The light is unevenly distributed, with brighter, concentrated regions and fainter, diffuse areas. These brighter regions may be star-forming knots or areas of higher stellar density. A faint tail-like structure extends from the main body, possibly a tidal feature resulting from gravitational interaction. Overall, the galaxy exhibits signs of significant dynamical activity.
