The galaxy presents as a system exhibiting possible ongoing interaction or a merger. There appear to be at least two distinct components visible.

The primary component exhibits a relatively smooth morphology, with a somewhat elliptical profile. It has a yellowish-orange hue, possibly indicating an older stellar population or significant dust obscuration.

A secondary component, located in close proximity to the first, displays a bluer color. The morphology of this component is less defined and somewhat irregular in shape. This color suggests a younger stellar population and ongoing star formation within this area.

There is a red point-source object located between these two components, but is probably a foreground star and not part of the galaxy itself. There is a slight tidal tail appearance to the upper component.

Overall, the system demonstrates a disturbed morphology indicative of either a recent merger or a strong gravitational interaction between the two components.
