This galaxy appears to be a spiral galaxy with a dominant central bulge. The bulge exhibits a smooth, concentrated light profile, suggesting an older stellar population. Fainter spiral arms emanate from the bulge, displaying a clumpy morphology indicative of active star formation regions. These star-forming regions appear redder in color. There also appears to be evidence of a possible minor disturbance in the disk. The overall shape of the galaxy is somewhat elongated, but it is primarily round in shape. 
