The observed galaxy presents as a spiral type, exhibiting well-defined spiral arms. These arms are moderately wound, tracing a path from the central bulge outwards. The central bulge is prominent, although not overly dominant in size relative to the disk. It is surrounded by a bright disk, indicative of significant stellar populations. The galaxy displays a slight hint of a bar-like structure extending from the center. The disk exhibits some asymmetry, potentially indicative of minor gravitational interactions or internal disturbances. Overall the morphology is largely undisturbed, with no major mergers, although there may be some minor disturbance. There are several spiral arms that begin close to the center and move away to the outer edge of the galaxy.
