This galaxy presents as a spiral galaxy, exhibiting a disk-like structure and spiral arms. The spiral arms are prominent, tracing a clear pattern extending from the central bulge. These arms appear fairly well-defined with a mixture of dust lanes and star-forming regions. There are at least two prominent spiral arms. The galaxy is observed at a relatively face-on orientation. The central bulge appears moderately sized in relation to the overall disk. The disk appears somewhat disturbed. There is no obvious strong bar feature. The galaxy does not appear to be undergoing a major merger or show evidence of strong tidal disturbances, though minor disturbances cannot be ruled out. There is evidence of active star formation within the spiral arms, indicated by the presence of HII regions along the arms.