The galaxy presents as a structured, albeit somewhat disturbed, system. The core exhibits a high degree of luminosity and a yellowish hue, suggesting an older stellar population. Surrounding this central region is an extended halo of lower surface brightness. There are hints of spiral structure, or possibly tidal arms or plumes, extending from the central bulge. These features appear asymmetric, implying potential gravitational interactions or past merger events. Some regions exhibit bluer colors, which could point to ongoing star formation. The overall morphology suggests a galaxy that is either in the process of merging or has experienced a recent interaction. The galaxy is of considerable mass and is likely actively forming stars.
