The galaxy appears to be a spiral galaxy, viewed at an angle between face-on and inclined. The disk shows evidence of spiral arm structure, although the resolution limits detailed tracing. The arms exhibit a patchy distribution of star formation regions, indicated by variations in color. The central bulge region appears moderately sized relative to the disk and exhibits a yellowish hue. The overall morphology suggests ongoing star formation. There is no obvious evidence of a strong bar structure, although a weak bar may be present. The galaxy does not exhibit signs of a major merger event, such as tidal tails or significant morphological disturbance, however there is some indication of minor disturbance.
