This galaxy exhibits a prominent disk structure. The spiral arms are well-defined, appearing predominantly as two distinct arms. The tightness of these arms varies, presenting a mix of tightly wound and more open structures. A bar feature appears to be present in the galaxy's central region, possibly a strong one. The bulge is of moderate size, not dominant, but neither particularly small. The galaxy's central region presents a somewhat yellowish hue, possibly indicative of an older stellar population, while the arms contain bluer regions, suggesting more recent star formation. Overall, the galaxy's form does not appear to be significantly disrupted, although some minor disturbances cannot be ruled out based on morphology. The galaxy shows evidence of star formation occurring within its spiral arms.
