The galaxy presents as a disk-like structure, viewed at an oblique angle. The central bulge appears yellowish-white, indicating a population of older stars. The outer disk regions exhibit a bluer hue, suggesting ongoing star formation. The galaxy shows no significant signs of major mergers or strong tidal disturbances, although subtle asymmetries may indicate minor interactions or internal dynamic processes. Overall, it appears to be a relatively well-defined spiral galaxy, with a moderate degree of internal star formation activity.
