The galaxy presents a discernible spiral structure. Arms are visible but not sharply defined. A central bulge region exhibits a brighter concentration of light, indicating a higher density of stars. The disk appears to have a slight inclination relative to the line of sight, presenting a mostly face-on view. Overall color appears to be largely composed of intermediate range wavelengths, which would seem to indicate a normal distribution of star ages throughout. There are slight disturbances visible, and they may be the sign of recent or ongoing interactions with another galaxy. A lack of strong tidal features, this disturbance does not appear to be the result of a major galactic merger.
