The observed galaxy presents as a spiral galaxy with distinct, albeit somewhat disorganized, spiral arm structures. The arms exhibit a flocculent morphology. The disk of the galaxy is viewed at a moderate inclination, not quite edge-on, which allows for observation of potential features within the disk. There is evidence of blue light concentration within the spiral arms, suggestive of ongoing star formation. A central bulge appears to be present, however it seems to be relatively small and difficult to discern within the overall disk. The galaxy's color profile indicates a relatively active star formation rate with a low mass, resulting in a very low specific star formation rate. It appears to be undergoing some form of gravitational interaction or disturbance, potentially a minor or major merger event. The presence of spiral arms, coupled with the observed disturbances, suggests the galaxy is dynamically active. A bar may exist within the central region, but it is difficult to confirm based solely on this image. Overall the system has a "featured" and "disk" fraction.
