The galaxy presents a primarily face-on orientation. A central bulge is visible, displaying a moderately concentrated luminosity profile. Spiral arms appear to emanate from the bulge region. The winding of these arms appears to be primarily of a medium and tight nature, with hints of a loose pattern as well. Two dominant arms can be visually identified, although it is possible that more arms exist but cannot be clearly distinguished. There is no indication of the presence of a significant bar structure. The galaxy exhibits a degree of disturbance in its morphology, suggesting a possible interaction. However, no clear signs of a merger are detected.
