The galaxy presents a disk-like morphology, observed at an angle approaching edge-on. Spiral arm structures are present, though not highly defined. A central bulge is visible but does not appear to dominate the overall structure; it is of moderate size relative to the disk. A bar-like structure is weakly suggested within the central region, though not definitively apparent. There is no obvious sign of major mergers; however, there may be a hint of minor disturbances in the disk. Star formation appears ongoing but at a low rate. Overall, the galaxy exhibits a somewhat smooth and regular appearance, characteristic of a late-type spiral galaxy.
