The object presents as a likely galaxy exhibiting a multi-component structure. The primary component is a bright, roughly circular, and smooth region dominating the overall light output. Adjacent to this primary component are two fainter, less defined regions extending along a somewhat linear trajectory. These fainter regions appear more diffuse and potentially connected to the primary structure.

The galaxy exhibits a yellowish-orange hue, suggesting a stellar population with a significant presence of evolved stars. There are no readily discernible spiral arms or prominent dust lanes visible, suggesting a morphology closer to elliptical or lenticular. The asymmetry and presence of multiple components suggest a galaxy undergoing or having undergone a merger or interaction with another galaxy. Further investigation is warranted to determine the nature of this interaction and the properties of each component.
