The galaxy appears to be undergoing a significant interaction with another galaxy, or potentially two distinct interactions. A primary, brighter component exhibits a smooth morphology, potentially an elliptical or lenticular galaxy viewed somewhat face-on. It displays a concentrated central bulge with a yellowish-white hue, indicating an older stellar population. 

A second, smaller component is visible adjacent to the main galaxy. This component presents a bluer color, which could signify ongoing star formation. This galaxy also appears to be less smooth, indicating it could be a late type, or spiral galaxy.

There is also an artifact in the image, though, so a third object in the image could be a false positive, and it is hard to interpret. 

Overall, the system exhibits signs of morphological disturbance, suggesting ongoing or recent gravitational interactions between two or three objects. Further investigation is necessary to determine if this is in fact three objects or just one, but the system is undergoing significant changes.
