The galaxy presents a complex morphology, appearing to be undergoing a significant interaction or merging event. A prominent, somewhat distorted disk is visible, exhibiting a bluish hue indicative of ongoing star formation. This disk does not appear to be perfectly edge-on or face-on. A yellow-shifted central bulge or a second galaxy appears distinct from the main disk. Evidence of tidal features or disturbances are visible, suggesting a recent or ongoing gravitational interaction. The overall structure indicates this is not a typical elliptical galaxy; rather, it displays characteristics of a disturbed spiral or irregular galaxy. The system is likely in a relatively active phase of star formation.
