The galaxy presents as a centrally concentrated object with a somewhat elliptical morphology. The core region is characterized by a bright, nearly white to yellow hue suggesting a population of older stars. A faint, diffuse halo surrounds the central bulge. The outer regions of the galaxy exhibit a bluer coloration. This is indicative of ongoing star formation within the galaxy. The galaxy lacks any distinct spiral arm structures or a prominent disk. There is a slight indication of disturbance in the outer halo suggesting a possible past minor merger event. Overall, it appears to be a relatively smooth galaxy.
