The galaxy presents as a relatively smooth, centralized structure. It exhibits a largely elliptical morphology, appearing nearly round. Faint color gradients are observable, shifting from a slightly bluer hue in the central region to a redder tone in the outer areas. There is no obvious spiral structure or distinct dust lanes evident in the image. The overall appearance suggests a minimal amount of ongoing star formation. There are no indications of major merger events, but the galaxy does show minor asymmetry, likely due to gravitational interactions.
