The galaxy presents as a roughly elliptical structure with a bright, concentrated central bulge. The bulge exhibits a yellowish hue, suggesting an older stellar population. Faint, bluish spiral arms appear to emanate from the central region, indicating the presence of ongoing star formation. These arms are not well-defined and display a somewhat patchy distribution. The overall color of the galaxy is slightly bluer than the central bulge, pointing towards a more mixed stellar population in the disk. The galaxy appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions, though there could be some minor disturbances in the disk. The morphology suggests a spiral galaxy with a dominant bulge component.
