The galaxy presents as a spiral type, viewed at a slight angle to face-on. The central bulge appears moderately sized and concentrated. Spiral arms are visible, demonstrating a somewhat open morphology. The bluer color of the arms, compared to the yellower hue of the central bulge, indicates active star formation regions within the arms. There is some evidence of a possible interaction or minor disturbance, as there may be a slight asymmetry within the outer disk structure. I do not detect a prominent central bar.
