The galaxy presents as a spiral type, with a noticeable disk structure. Evidence of spiral arms is visible, albeit somewhat disrupted. The color suggests active star formation, particularly in the spiral arms which show a distinct blue hue, indicating the presence of young, hot stars. There appears to be some evidence of a bar structure within the central region, but the arms are not clearly defined, possibly due to dust obscuration or tidal disruption. The bulge is difficult to discern, suggesting that it is either small or not prominent. The galaxy exhibits irregular features, potentially indicative of an ongoing or recent interaction or merger with another galaxy. There appears to be a notable amount of tidal tail, and it is likely interacting with another galaxy.
