The observed galaxy presents as a spiral galaxy with a relatively small bulge, viewed at a significant inclination. The galaxy is dominated by a disk. Two prominent spiral arms can be discerned. Evidence suggests a bar structure is present within the galaxy, potentially extending across a considerable portion of the central region. The spiral arms exhibit a moderately tight winding pattern. Overall, the galaxy does not appear to be undergoing any significant merging events, though minor tidal disturbance cannot be ruled out. There is a low rate of star formation.
