This galaxy exhibits a disk-like morphology, but appears disturbed. It has a blue hue, which indicates the presence of young, hot stars and active star formation regions. A significant portion of the galaxy exhibits a smoother, less defined structure, potentially indicating an older stellar population or the aftermath of a merger event. There is evidence of tidal features or minor disturbances; these are suggestive of gravitational interactions with another galaxy or recent internal dynamical activity. Overall, the galaxy shows signs of past or ongoing interaction, potentially influencing its star formation rate and morphological features.
