The galaxy exhibits an irregular morphology, appearing as a disturbed system indicative of an ongoing or recent interaction or merger event. Two distinct, luminous components can be observed, suggesting the presence of two galactic nuclei or highly concentrated regions of star formation. There is no obvious disk structure, with a dominant smooth component. The overall color of the galaxy is yellowish-white, with some regions tending towards a more reddish hue, indicating a likely intermediate age stellar population, with older components dominating the light. The shape is elongated with a moderate level of roundness, with one end slightly more diffuse. A high likelihood of merger activity or a significant disturbance to the system's morphology is supported by these visual features.
