This galaxy exhibits a complex morphology, displaying characteristics of an ongoing or recent interaction or merger. A distinct, compact, and relatively circular structure is visible, exhibiting a bluish hue, potentially indicating a region of active star formation. Connected to this structure is an elongated tidal tail or arm. This arm displays a diffuse, lower surface brightness than the main component. The arm possesses a curved structure. There appears to be a disruption in the overall smooth distribution of light, suggesting ongoing gravitational disturbances within the system. The overall structure is neither purely elliptical nor clearly spiral, thus lending credence to the possibility of a disturbed morphology from a merger.
