This galaxy exhibits a generally smooth morphology, with a somewhat elliptical shape. The light is highly concentrated towards the center, exhibiting a bright, yellowish core that could indicate a significant population of older stars. Moving outward from the center, the luminosity gradually decreases. There are some subtle color variations in the outer regions, hinting at possible faint spiral arms or features, though they are not well-defined. There is a lack of prominent dust lanes, which further supports a classification as an early-type spiral or potentially an elliptical galaxy. There are no obvious signs of a major ongoing merger or strong tidal disturbances, although there may be some minor asymmetry suggesting a past interaction or minor disturbance.
