The galaxy presents a disk-like structure with noticeable features. It is not perfectly smooth, showing some evidence of disturbance or structure within the disk, with more than half of measured votes being positive. The galaxy is not seen perfectly edge-on. The central bulge is prominent and has a bright, concentrated luminosity. A faint, blue-ish spiral arm structure is visible extending outwards from the bulge. There is a suggestion of ongoing or recent star formation, inferred from the galaxy's color. Overall, the galaxy appears relatively isolated, and the color information suggests relatively low levels of star formation. There is evidence of minor disturbances.
