The galaxy appears to be in a late-stage merger or strong interaction with another galaxy. Two distinct luminous cores are visible, each surrounded by a more diffuse, elongated envelope of light. These envelopes seem to be connected by a faint bridge of material, suggestive of tidal forces acting between the galaxies. The galaxy pair exhibits a relatively smooth, blended morphology overall, though there is some evidence of disturbed structure and asymmetry. Both components display a yellowish hue, suggesting an older stellar population with relatively little ongoing star formation. The overall shape of the system deviates significantly from a regular elliptical or spiral structure.
