The galaxy presents a face-on spiral morphology. A prominent, moderately sized bulge dominates the central region, exhibiting a yellowish-white hue, potentially indicating an older stellar population. Faint, tightly wound spiral arms emanate from the bulge, displaying a bluer tint, suggestive of ongoing star formation. The overall structure is well-defined, with a relatively smooth disk component. There are slight indications of disturbances or asymmetries in the outer regions of the disk, possibly suggesting past minor interactions or merging events. A faint bar structure may be present, although its definition is uncertain.
