The galaxy exhibits a complex morphology indicative of an ongoing merger event. Two distinct nuclei are visible. The primary nucleus presents a smoother, more concentrated light profile with a yellowish hue, suggesting an older stellar population. The secondary nucleus is less defined, appearing bluer in color, possibly indicating more recent star formation activity.

A faint tidal tail or bridge of material appears to connect the two nuclei, supporting the merger hypothesis. The overall shape is disturbed and asymmetrical. The galaxy's light distribution is concentrated in the central region, although faint extensions can be seen. Evidence of substantial tidal disruption is observed.
