The galaxy presents as a spiral type, observed at an angle significantly inclined from face-on but not quite edge-on. It exhibits a disk-like morphology with distinct spiral arm structures visible, possessing a noticeable, but not overly prominent central bulge region. The spiral arms are well-defined and appear tightly wound around the central bulge. The arm structure suggests a grand design type spiral with two major arms. Star formation regions are readily visible along the spiral arms. The disk shows no signs of major tidal distortions or ongoing mergers, although some minor irregularities may be present. There may be a weak bar structure. Overall, the galaxy appears to be a relatively isolated, well-formed spiral galaxy.