The galaxy presents as a singular, relatively smooth object with a slight elongation. It appears to be in the process of merging or interacting with another galaxy, as evidenced by the dual-core morphology. One core appears bluer in color, while the other is redder, potentially indicating differing stellar populations or dust content between the two components. There is a lack of distinct spiral arm structures or other prominent features typically associated with undisturbed disk galaxies. The overall structure suggests a significant degree of morphological disturbance, likely due to the ongoing interaction. The dominant component of light is concentrated in the central regions, suggesting a high degree of central mass concentration.
