The galaxy presents as a spiral with a prominent bulge. The spiral arms are tightly wound and extend from the central bulge. There are areas of intense star formation evident within the spiral arms, appearing as clumpy regions. A bar structure appears to be present, bisecting the central bulge. The galaxy appears to be undergoing some type of interaction or disturbance, with irregularities in the arm structure. The bulge contributes a significant portion to the overall luminosity.
