The galaxy presents a generally smooth appearance, with a hint of internal structure. It appears to be an elliptical galaxy, showing an elongated shape rather than a distinct spiral pattern. The central region shows increased brightness, indicating a higher concentration of stars, possibly housing a supermassive black hole. The color profile suggests a population of older stars, with the overall hue trending toward the redder end of the spectrum. There is a subtle indication of a possible tidal feature or minor disturbance on one side of the galaxy, hinting at a past interaction with another galaxy or a minor merger event.
