The galaxy appears to be a spiral galaxy, viewed at an angle that is neither perfectly face-on nor edge-on. The disk is clearly visible. The spiral arms are tightly wound, with significant star formation occuring within. The central bulge is apparent but not dominant, and the lack of pronounced dust lanes suggest it is relatively small compared to the overall disk. There is no clear indication of a strong bar structure. The galaxy exhibits a bluer hue in the disk and spiral arms indicating current active star formation, with a slightly redder core, potentially indicative of an older stellar population. The overall morphology suggests a moderate spiral galaxy.
