The galaxy presents as a singular, somewhat elliptical, smooth-appearing object. Its core exhibits a strong, concentrated luminosity, suggesting a significant stellar density or active galactic nucleus. The primary color is a warm yellow/orange hue, indicative of an older stellar population dominating the light output. A slightly fainter, more diffuse area is visible near the core, potentially signifying a secondary center of activity or a less concentrated region of star formation with a hint of bluer light mixed in. Overall, there are visual indications of a system undergoing, or having undergone, a significant interaction or merger event, given the relatively unstructured morphology.
