The galaxy exhibits a spiral morphology, with a prominent central bulge region characterized by a yellow-white hue. This bulge gradually transitions into a disk with defined spiral arms. These arms appear tightly wound and are composed of a mix of blue and white regions, likely indicative of active star formation. Some regions of the arms closer to the bulge appear to have some redder hues. The galaxy displays a bar structure and there are regions of disturbance indicating possible past minor merging events. It is not oriented perfectly face-on, but rather has a slight inclination, which is also indicated by the elliptical appearance of the bulge and disk. Overall, the galaxy presents as a well-formed spiral structure, characterized by a mixture of old and young stellar populations.
