The galaxy exhibits a disturbed morphology, indicative of an ongoing or recent interaction. The central region shows a concentration of light, possibly a bulge, but it's irregular and disrupted. Faint, diffuse tidal features are visible, extending outwards from the main body of the galaxy. Blue-ish knot structures are visible within the extended tails, which possibly indicate regions of active star formation triggered by the interaction. The central region of the galaxy also has a yellowish hue. There are no clear spiral arm structures. The overall impression is of a galaxy undergoing a significant gravitational disturbance.
