The galaxy presents as a fairly symmetrical, centrally concentrated object, likely an elliptical or lenticular galaxy given its smooth morphology. The galaxy core exhibits a bright, yellowish-white hue, indicating a population of older, less massive stars. Moving outward from the core, the color shifts to a slightly bluer tone, hinting at a possible population of younger stars within the outer regions. The galaxy appears moderately sized with a slightly blurred edge and faint outer regions, suggesting it is at a considerable distance. The general form shows signs of potential minor gravitational disturbances, perhaps an ongoing minor merger event.
