The observed galaxy presents an elliptical morphology, exhibiting a smooth light distribution that gradually decreases in intensity from the center outwards. It appears to be tilted, with the major axis being approximately twice the length of the minor axis. The core region is bright and concentrated, with a yellowish-white hue that suggests a population of older stars. There are no distinct spiral arms or significant dust lanes visible. There is a faint, elongated disk, mostly round in nature, showing a slight blueish tone. The outer edges are somewhat diffuse. No signs of recent merging events are easily seen. 
