The galaxy presents a morphology suggestive of an ongoing or recent merger event. Two distinct components are visible. The brighter component exhibits a relatively smooth and concentrated light distribution, with a bright core and a gradual decrease in luminosity outwards, suggesting an elliptical morphology. The second component appears to be a more diffuse, disk-like structure with a less concentrated light profile and a noticeable reddish hue.

There may be some signs of tidal disturbance surrounding the galaxy, though the image resolution makes it difficult to definitively assess the presence of tidal tails or bridges. There are subtle extensions of light emanating from the galaxy, hinting at interactions. However, this could also be noise. Further investigation with higher-resolution imaging and spectroscopic data would be required to characterize the merger stage of the galaxy.
