The galaxy presents as a generally smooth, elliptical structure with no prominent spiral arms or bar. The morphology appears largely spheroidal, exhibiting a high degree of central concentration with a gradual decrease in luminosity moving outward from the core. There is an obvious yellow hue at the core, suggestive of an older stellar population, while the outer regions exhibit bluer tints. No signs of ongoing or recent major merger events can be identified. The lack of dust lanes or other obscuring features is apparent. The galaxy has a relatively round shape and no signs of significant disturbance or interaction are visible.