The galaxy appears to be disk-shaped when viewed from its current angle. It presents a central bulge that shines very brightly, dominating the galaxy's overall luminosity. The bulge region appears symmetrical. Surrounding this central condensation is a fainter, more diffuse disk. The disk structure is relatively smooth, with a notable lack of defined spiral arms. There is a slight indication of a ring-like structure around the central bulge. There is an indication of slight morphological disturbance but not in the form of mergers or distinct structures. The dominant color of the galaxy appears to be light blue transitioning to green, with red in the center. This suggests a population of younger stars, particularly in the bulge region, though there are also some older stellar populations present.
