The galaxy exhibits a spiral structure, with tightly wound arms emanating from a prominent central bulge. The arms are well-defined and display a notable degree of symmetry, indicating a relatively undisturbed morphology. A bar-like feature appears to be present, extending across the central region of the galaxy. The color gradient suggests a higher concentration of older stars in the bulge, with bluer regions apparent within the spiral arms, possibly indicating regions of active star formation. The galaxy is moderately inclined with respect to our line of sight, offering a partial view of its disk structure. There appears to be some sort of disturbance present within the galaxy as well, but difficult to ascertain due to the image quality.
