The galaxy appears to be a spiral type, though possibly seen at an oblique angle. A significant tidal tail of stellar material extends from the main galactic body. The core region exhibits a bright, almost unresolved morphology. A disk component is faintly visible, with bluer colors than the main body. The blueish coloration suggests more recent star formation activity within the disk region. The color of the tail appears redder than the center, indicating an older stellar population. The galaxy exhibits a distinct disturbance or asymmetry, likely due to a minor interaction with another galactic object.
