The galaxy exhibits a morphology consistent with a major merger event. The light distribution appears disturbed, with an irregular shape that does not conform to a simple elliptical or spiral structure. There is evidence of two distinct nuclei, which are the brightest regions within the galaxy, indicating that the merger process is ongoing. 

The primary color is yellowish-white. The overall structure is diffuse and lacks sharp features, suggesting a well-mixed stellar population. While the galaxy shows evidence of star formation, it is occurring at a modest rate. The galaxy is relatively massive.
