The galaxy presents a disturbed morphology, suggesting an ongoing or recent interaction. A prominent tidal tail extends outwards, exhibiting a bluish hue, possibly indicating a region of active star formation. The main body of the galaxy appears to be disk-like, although it has a warped or irregular shape. There is some yellow or reddish dust within the disk. The overall structure is complex, with no readily apparent spiral arm structure visible. The light distribution is concentrated in the central regions, but is asymmetric, with distinct features indicative of gravitational disturbances. The galaxy’s apparent orientation is close to edge-on. A large fraction of the galaxy seems to consist of this warped or disturbed disk and tidal tail.
