The galaxy presents with a complex morphology, seemingly undergoing an active merger. The central region is characterized by a bright, concentrated luminosity, appearing almost as if there are two distinct nuclei or condensations. This region exhibits a yellowish-white color, suggestive of a significant population of older stars or potentially dust obscuration. Faint blue tendrils extend outward from the central region, indicating possible tidal tails or disrupted spiral arm structures. These features are consistent with ongoing gravitational interactions. There appears to be some dust present within the galaxy, especially given that the magnitude is highest in the G band (blue light) and lowest in the Z band (far-red light). There is no apparent ordered structure such as a spiral disk or defined elliptical shape.
