The galaxy presents a morphology consistent with a spiral galaxy viewed at a moderate inclination angle. Two prominent spiral arms emanate from the central region, appearing relatively tightly wound. There's an indication of a central bulge, with an intermediate size relative to the overall disk. The arms exhibit a granular texture indicative of regions of star formation. The galaxy is not perfectly symmetrical, displaying slight irregularities possibly due to minor gravitational interactions. The galaxy appears to be at a distance where its features are moderately resolved, allowing for the discernment of its spiral structure.
