The galaxy appears to be a relatively compact, disk-shaped structure. The central bulge is bright and centrally concentrated. The disk component is visible as a fainter, extended structure surrounding the bulge, with the galaxy being more luminous toward the center, indicative of a higher stellar density there. The disk's orientation is close to edge-on, obscuring any spiral arm features if present. There are very small visual disturbances, perhaps hints of a minor merger. The overall color suggests an actively star-forming environment, with bluer hues present at the outer regions of the disk, indicating the presence of younger, hotter stars.
