This galaxy presents as a spiral type, viewed at an oblique angle, not quite edge-on. The central bulge is prominent, exhibiting a yellowish-white hue, suggesting an older stellar population. This bright bulge appears to be a moderate size relative to the rest of the disk. Faint spiral arms are visible extending from the central bulge. There are hints of a disk component with slightly bluer colors. The disk shows some features, but these are not perfectly uniform or smooth. There is no major apparent disturbance in the galaxy, indicating that it is not undergoing a major merger. However, the galaxy shows mild irregularities which indicate a minor disturbance could be occurring. There does not seem to be a bar structure in this image.
