The galaxy appears to be a spiral galaxy seen at an oblique angle. There is a central bulge of moderate brightness. Traces of spiral arm structure are visible, though somewhat disrupted. The disk of the galaxy presents an intermediate ellipticity, exhibiting an elongated shape but not highly flattened. The color profile suggests a moderate amount of on-going star formation, as indicated by the blue hue interspersed within the spiral arms and a redder bulge. The overall morphology hints at possible past or ongoing minor gravitational interactions, as evidenced by the irregular arm structure. The galaxy does not appear to be a major merger event, nor does it appear smooth and featureless.
