The galaxy presents as a slightly tilted, disk-shaped system. There is a prominent, bright central bulge that appears roughly elliptical in shape. Faint spiral arms can be observed in the disk; they appear relatively tightly wound. The disk exhibits a slightly mottled texture, suggesting some degree of star formation activity. The color profile indicates a blueish tinge in the disk, characteristic of a somewhat higher concentration of younger, hotter stars. The overall color indicates a galaxy that contains both young and old stars. The galaxy is slightly elongated with a bar structure in the central region. There are two spiral arms. One goes up towards the top, then curls in and down towards the bottom left of the central region. The second starts on the bottom region of the central area and spirals up and out. There does not appear to be any signs of ongoing major merger events or strong tidal interactions.
