The galaxy presents as a multi-component system, seemingly undergoing a significant interaction or merger. The primary component appears as a largely amorphous elliptical or lenticular galaxy, exhibiting a smooth texture and a concentrated yellowish hue, suggesting a population of older stars. Immediately adjacent is a less defined region with a distinctly blueish tint, possibly indicating a region of active star formation. There is the suggestion of tidal features or distortions in the system's morphology, hinting at gravitational interactions. Overall, the system lacks a clear, defined structure, possibly indicating an advanced stage of merging or disturbance.
