This galaxy presents as a spiral galaxy with a prominent central bulge. The spiral arms are tightly wound, exhibiting a relatively high degree of symmetry. The color of the bulge appears more yellowish, suggesting an older stellar population, while the spiral arms display a bluer hue, indicating the presence of younger, hotter stars and ongoing star formation. The galaxy appears to be actively forming stars within the spiral arms. There are indications of a bar structure. The disk is viewed at a moderate angle, not quite face-on nor edge-on. There appears to be a disturbance to the morphology of the galaxy, but no indication of a major merger with another galaxy.
