The galaxy exhibits a clear spiral structure. The arms appear to be fairly well-defined, with a medium winding pattern. Evidence suggests the presence of two prominent spiral arms. A bar structure appears prominent across the central bulge of the galaxy, moderately obscuring the center of the bulge. The bulge size is moderately pronounced. Some asymmetries and irregularities are visible in the spiral arm structure, possibly indicating minor gravitational interaction or disturbance. The disk is oriented close to face-on, though it may have a slight tilt to our line of sight. The presence of significant star formation regions within the spiral arms can be inferred from the bluer colors observed within those areas, particularly compared to the redder hue of the bulge. There is no indication of strong merging, though tidal features suggest the possibility of a minor disturbance.
