The galaxy presents as a spiral type, viewed at an angle slightly offset from face-on. The central bulge appears moderately sized and exhibits a bright, yellowish-white hue. The disk is the dominant feature, with evidence of spiral arm structure. These arms are tightly wound and their exact number is difficult to ascertain due to the viewing angle. The presence of a weak bar feature cannot be ruled out. The arms show a bluer color, possibly indicating ongoing star formation. The galaxy appears relatively undisturbed, with no readily apparent signs of a major merger event, although there might be some indication of a minor tidal disturbance.
