The galaxy presents a morphology indicative of an ongoing or recent merger event. Two distinct luminous components are visible, each possessing a relatively smooth, elliptical-like structure. These components appear to be interacting gravitationally. The primary luminous component exhibits a slightly more concentrated and yellow color, while the other is less concentrated with a slightly redder hue. There is evidence of tidal features or disturbances; the overall shape is not perfectly elliptical, with some asymmetry suggesting gravitational interactions. The light distribution is relatively diffuse, lacking strong central concentration apart from the two core components. Based on its red color, it likely has a relatively high mass with little star formation. There are no distinct spiral arms or dust lanes visible in this image.
