The galaxy presents as a complex system, likely undergoing a merging event. The primary component exhibits a relatively smooth morphology, though some irregularities are visible. A secondary, smaller component appears connected via a bridge of diffuse light, suggesting tidal interactions. Both components display a bluish hue, indicative of ongoing star formation. The overall structure is irregular and lacks a defined shape, consistent with a disturbed system. There are some indications of potential dust lanes or differential reddening within the larger component. The extent of tidal tails or other debris is not immediately clear, but some faint extensions hint at past interactions. The system appears relatively compact in angular size.
