The galaxy appears to be an interacting system, with two distinct components. The primary component exhibits a smoother, more concentrated light profile, potentially indicative of an early-type galaxy or the bulge of a spiral galaxy. It presents a yellowish hue, suggesting an older stellar population with fewer ongoing star formation events.

The secondary component is more diffuse and displays a bluer color. This indicates a younger stellar population and active star formation. Its morphology appears somewhat disturbed and possibly tidal in nature, suggesting a connection to the gravitational interaction with the primary component.

The overall shape of the system is elongated, with a cigar-shaped morphology. There appears to be a potential bridge of material, however faint, connecting the two components. This connection is supportive evidence of an ongoing interaction. There is a possibility that this system will eventually merge, which would lead to a new stage in its evolution.
