This galaxy appears to be a spiral galaxy with a relatively bright central bulge. The spiral arms are well-defined and extend outwards from the bulge in a sweeping pattern. Two main arms are prominently visible. The arms display a noticeable degree of star formation, indicated by their slightly bluer color compared to the bulge. There appears to be a bar-like structure crossing the center of the galaxy, which could influence the shape of the spiral arms. The disk is observed face-on. The overall color suggests it is an intermediate type spiral galaxy, not extremely blue or red. No signs of major mergers are visible, although some minor disturbances or irregularities within the arms could be indicative of smaller interactions. The galaxy seems to be well-defined, indicating a mature, stable system.
