The galaxy presents as an elongated, cigar-shaped structure. Its overall color is a soft bluish-white, indicative of a population of relatively young, hot stars. The central region exhibits a greater concentration of light, suggesting a bulge possibly composed of older stellar populations or a supermassive black hole. There are some faint features of a spiral arm-like structure with subtle irregularities within the main body of the galaxy. Based on its morphology, it appears to be undergoing only minor gravitational interactions or disturbances. There is faint dust that appears to be embedded within this spiral structure.
