The galaxy exhibits a morphology suggesting a system undergoing a potential merger or strong interaction. Two distinct components are visible.

The larger component presents a smoother, more diffuse appearance with a relatively concentrated central region. The light distribution appears elliptical with a high Sersic index suggesting a concentrated core. The other, smaller component appears more compact and less luminous, exhibiting a more defined core. Tidal features or distortions are present, which are indicative of gravitational interaction. A faint bridge of light appears to connect the two components suggesting an active interaction. The galaxy shows evidence of both ongoing and recent star formation, indicated by the color gradients across the galaxy, suggesting that this interaction is stirring up star formation within the system.
