The galaxy presents a generally smooth, elliptical morphology. Its core appears bright and concentrated, suggesting a significant stellar density. The light distribution is more concentrated toward the center, with a radial falloff in surface brightness typical of elliptical galaxies. The galaxy displays an overall yellow-orange hue, indicating an older stellar population. The absence of prominent spiral arms or significant dust lanes supports a classification as an elliptical galaxy. There may be a minor asymmetry or tidal feature, indicative of a past interaction or minor merger event, but it is not highly pronounced. Based on the color and morphology, star formation is likely to be relatively low within the galaxy.
