The galaxy exhibits a spiral structure, viewed at an angle that is neither fully face-on nor edge-on. The spiral arms are evident, displaying a patchy distribution of light, suggesting active star formation regions within. There is a slight color variation across the galaxy, with bluer hues concentrated in the arms and a more yellowish or reddish tone towards the central region. The central bulge is not very prominent. The overall morphology indicates an actively star-forming spiral galaxy undergoing possible interactions. It appears as though there may be a disturbance in the morphology, which could be caused by either a tidal interaction or recent galaxy merger. There is no single, dominant nucleus, but rather two dimmer areas that may be a sign of a double nucleus of two interacting galaxies.
