The galaxy exhibits a distinct spiral morphology. It possesses a bright, concentrated central bulge that appears yellowish-white in color, surrounded by a relatively tightly wound spiral arm structure. The spiral arms themselves are somewhat patchy, displaying a blue hue indicative of ongoing star formation regions. The disk of the galaxy appears to be relatively face-on, allowing for a clear view of the spiral structure. The galaxy does not appear to be undergoing any major merging events, although there is the possibility of some minor disturbances within the disk. The spiral arms appear to be composed of numerous star-forming regions, contributing to their distinct color and texture. There is no strong bar structure apparent. The ratio of the semi-minor to semi-major axis of the outer disk shows that the galaxy disk is fairly circular.
