The galaxy appears to be a spiral galaxy, viewed at a slight angle from face-on. It exhibits a prominent disk structure with well-defined spiral arms. The arms appear tightly wound. The central bulge is relatively small and compact, displaying a yellowish-orange hue, which might indicate an older stellar population within the bulge. The spiral arms exhibit a bluer color, suggesting the presence of younger, hotter stars and ongoing star formation. There are two spiral arms that dominate the shape of the galaxy. There appears to be no signs of significant tidal disturbances or major merger events. The overall structure suggests a relatively undisturbed and mature spiral galaxy. There is a faint object to the left that may be a smaller galaxy in orbit, or a foreground or background object. There is evidence of a bar structure within the central region, though it is not particularly strong.
