The galaxy presents a clear spiral structure. Two distinct spiral arms emanate from a central bulge. These arms appear somewhat loosely wound and extend a significant distance from the core. The color gradient suggests active star formation within the spiral arms, showing a blueish-white hue, contrasting with the yellower color of the central bulge, which likely indicates an older stellar population. There is a hint of a bar-like structure within the central region, but it is not prominently defined. The overall morphology suggests a disk-dominated galaxy, seen from a near face-on perspective, with no major signs of ongoing mergers or significant disturbances in its structure. The galaxy seems to be isolated, with no nearby companions visibly interacting with it.
