The galaxy exhibits a flattened, disk-like structure with a central bulge. There is a subtle degree of internal structure, suggestive of spiral arm features, though these are not sharply defined, the galaxy likely being in the transition between a spiral galaxy and a lenticular galaxy. The galaxy has a generally smooth appearance. The color gradient suggests a relatively uniform stellar population throughout the galaxy, with a slight increase in bluer wavelengths in the outer disk. The inclination suggests that the galaxy is not viewed completely edge-on, which allows for observations of the disk structure. There is a small chance it may be experiencing a minor disturbance or merger event, but that's likely not the case. Overall, the galaxy appears relatively undisturbed, and appears to be mostly dominated by older stellar populations, indicating suppressed star formation.