This galaxy presents a relatively compact appearance. It exhibits a central, bright, smoothly distributed core. Surrounding this central region is a less luminous, more diffuse halo. There is an irregular, somewhat lumpy structure observed in the outer regions of the galaxy. The color distribution suggests a bluer central region, possibly indicative of younger stellar populations or active star formation, while the outer regions display a redder hue. There may be some ongoing minor disturbance.
