The galaxy presents as a flattened, disk-like structure oriented approximately horizontally in the frame. A slight bulge is perceptible at the center, although it is not strongly pronounced. The color gradient suggests a possible difference in stellar populations between the central region and the outer disk, the core exhibiting a slightly more yellow hue, while the outer regions appear bluer. The disk structure appears to be relatively smooth with some faint disturbances, but does not have well-defined spiral arms. There are no indications of a strong interaction or major merger events. Overall, the galaxy is most likely a spiral galaxy, but without a clear spiral structure.
