The galaxy presents a relatively smooth and rounded appearance, suggesting it is likely an elliptical galaxy or a lenticular galaxy seen face-on. There is a concentration of light in the center, indicating a nucleus that may contain a supermassive black hole. The galaxy exhibits a color gradient, transitioning from a yellowish-white core to a redder outer halo. This color suggests an older stellar population, particularly within the core, with progressively younger stars residing further out. No distinct spiral arms or features indicative of active star formation are visible within the image. The high degree of smoothness and lack of asymmetrical features imply that the galaxy has undergone minimal recent interactions or mergers. There is no morphological indication of prominent dust lanes. The general roundness and lack of significant disturbances suggest it has largely settled into a stable structure.
