The galaxy appears as a dual-core system, or possibly two galaxies in the process of merging. Both components present with a relatively smooth, elliptical morphology. The larger, primary component exhibits a yellow-orange hue, suggesting an older stellar population and potentially a lower rate of active star formation. A distinct red tidal feature or dust lane is observed extending between the two components. The smaller component is rounder in appearance, with a yellower core. It is not clear whether this is simply the effect of the image processing or the properties of the galaxy itself. Based on the morphology, it would likely be classified as an early-type galaxy. Further spectroscopic analysis is required to determine its precise redshift, stellar population characteristics, and the nature of any ongoing interactions or merger processes.
