The galaxy exhibits a disturbed morphology, appearing to be the product of a merger. The primary structure consists of two distinct luminous components: a more compact, yellowish-white core region, and a bluer, less concentrated region located below it. These regions are connected by a faint, diffuse bridge of light. The overall shape is irregular, lacking a clear spiral arm structure or elliptical form. There is evidence of tidal features or streamers extending outwards, particularly in the upper area, indicating ongoing gravitational interaction. The galaxy displays a wide range of colors across its structure, suggesting varying stellar populations and star formation rates.
