The galaxy presents as a system comprised of two distinct components. The primary component exhibits an overall elliptical morphology. Its light profile appears smooth and concentrated towards the center, indicating an older stellar population. The color is yellowish-orange, suggesting a lack of significant ongoing star formation and a redder population of evolved stars.

A second, smaller and less luminous component is located in proximity to the primary galaxy. It's color is bluer. This secondary component appears more irregular in shape, potentially indicating a disturbed morphology. This configuration suggests a possible interaction or merger event. No prominent tidal features are discernible in the immediate vicinity.
