The galaxy exhibits a prominent disk structure. The majority of the light appears to be concentrated in a defined central region with a moderate-sized bulge, which is bright and appears relatively smooth. The spiral arms are tightly wound and show a propensity for multiple distinct arm segments. The color gradients suggest ongoing star formation within the disk, with bluer regions tracing the spiral arms, contrasting with the yellowish hue of the central bulge, likely indicative of an older stellar population. There appears to be no sign of major interactions or mergers. The overall morphology is consistent with a late-type spiral galaxy.
