The galaxy presents a complex morphological structure, likely undergoing a merging process. The system appears to consist of two main components: a larger, more diffuse, elliptical-like structure, and a smaller, bluer, disk-like component. The elliptical-like component exhibits a smoother light distribution, suggesting a population of older stars. The disk-like component, displaying a bluer hue, hints at ongoing star formation activity within its structure. Evident visual disturbances are present, including tidal features, which suggests gravitational interactions between the two components are present, indicative of a merger in progress. The system appears to be elongated, with an intermediate level of roundness. Overall, the morphology is suggestive of a galactic system in transition, influenced by merging dynamics.
