The galaxy presents as a spiral galaxy with a prominent disk structure. The spiral arms appear somewhat tightly wound around the central bulge. The bulge itself seems relatively small in comparison to the overall disk size, with the prominence of the spiral arm features suggesting a later-type classification. Some segments of the spiral arms exhibit a clumpy morphology, indicative of active star formation regions. Dust lanes can be inferred, obscuring the light from stars within the arms. There are no obvious signs of major merger activity. The galaxy is relatively blue in color suggesting some presence of younger stars. The galaxy appears to be significantly inclined with respect to our line of sight but is not fully edge on. The overall shape appears somewhat elliptical.
