The galaxy presents an elliptical morphology, appearing generally smooth and centrally concentrated. A bright, yellowish core dominates the galaxy's appearance, suggesting a significant population of older stars. There is no discernible spiral structure or dust lanes present. The color suggests a relatively passive galaxy with limited ongoing star formation, although subtle color variations hint at some lower levels of more recent activity. The outer regions of the galaxy exhibit a gradual decrease in luminosity. There is a slight suggestion of a tidal feature or minor disturbance in the structure. Overall, the galaxy appears to be a massive, relatively evolved system.
