The galaxy appears to be in the process of merging or undergoing a significant interaction. There are two distinct, luminous cores visible, suggesting either two galaxies in the process of coalescing, or one galaxy with a highly disturbed morphology resulting in a double nucleus. The overall color is predominantly yellow-orange, indicating a population of older stars and a relatively low rate of ongoing star formation. The shape of the system is irregular and lacks any clear spiral or elliptical structure. There is evidence of tidal features, though not pronounced, hinting at gravitational disturbances caused by the ongoing interaction. The light is relatively smooth, indicating the main component of the galaxy is a bulge and halo.
