The galaxy presents a relatively smooth and featureless morphology, suggesting a classification as an elliptical galaxy. Its overall shape appears slightly elongated, but largely rounded. The central region exhibits a high concentration of light, appearing bright and yellowish, indicative of an older stellar population. Progressing outward from the core, the light intensity gradually diminishes. The outer regions display a bluish hue, hinting at the presence of some younger stars or ongoing star formation, although this seems subdued. There appears to be a very minor disturbance of structure, suggesting some past interaction, but no major ongoing merger events are visibly apparent. Overall, the galaxy seems to be a massive system, with a relatively low rate of star formation.
