The galaxy presents a largely smooth and rounded morphology. The central region exhibits a high concentration of light, appearing a yellowish hue, indicative of an older stellar population. Moving outward from the center, the galaxy's light gradually diffuses into a less defined, more extended halo. There is a slight elongation or asymmetry in the outer regions but the overall appearance is largely elliptical. There are no readily apparent spiral arm structures or significant dust lanes visible in this image. The smoothness and color suggest a relatively quiescent galaxy, possibly an elliptical galaxy or a lenticular galaxy viewed face-on. Minor disturbances cannot be ruled out, but the overall structure suggests the galaxy is not currently undergoing a major merger event.
