The galaxy presents as a spiral type, viewed at a relatively face-on angle. It exhibits a central bulge that appears moderately sized and luminous, transitioning smoothly into the surrounding disk. The spiral arms are well-defined, with a noticeable winding pattern, appearing moderately tight. At least three arms are discernable, tracing outward from the core. The arm structures seem to be interspersed with regions of both heightened star formation and dust obscuration, giving it a textured look. The overall appearance is not suggestive of a major merger event, but there might be some minor disturbances evident in the morphology. There is an indication of a weak bar-like feature that exists in the galactic center, but this is quite faint. The galactic disk appears moderately inclined.