This galaxy presents as a relatively smooth, elliptical-like structure. Its overall color appears to be a yellow-red hue, indicative of an older stellar population with lower star formation rates. The central region is brighter and more concentrated, suggesting a higher density of stars and potentially a supermassive black hole at the core. No distinct spiral arms or features of active star formation are visually apparent. There might be a subtle flattening, but not enough to indicate a disk galaxy. The round shape is quite regular and shows very little indication of being a galaxy currently involved in any type of merger activity. The observed characteristics point toward it being an early-type galaxy with minimal ongoing star formation.
