The galaxy exhibits a spiral morphology, characterized by prominent arms extending from a central bulge. These spiral arms are well-defined and relatively tightly wound. The central bulge appears moderately sized with a yellowish color indicative of an older stellar population. Patches of blue are seen scattered throughout the arms, suggesting regions of active star formation. The disk shows a slight inclination, offering a partial view of the galactic structure. There may be some level of disturbance in the disk, but no major interactions are apparent.
