The observed galaxy presents a spiral morphology, characterized by prominent spiral arms emanating from a central bulge. The spiral arms exhibit a moderate winding, appearing neither tightly wound nor excessively loose. There appears to be 3 or 4 spiral arms. The arms are defined by regions of intense blue star formation. The central bulge appears relatively small compared to the overall disk size. No strong bar structure is obviously apparent, although a subtle, weak bar might be present. The galaxy does not appear to be significantly disturbed or undergoing a major merger, although there are minor irregularities that suggest possible interaction with another galaxy. The galaxy is observed at a redshift indicating a relatively nearby location. The low redshift indicates a low velocity. The galaxy is not observed edge on, instead closer to face on. The Bulge is small compared to the rest of the galaxy.
