The galaxy exhibits a distinct spiral structure, with well-defined arms emanating from a central bulge. These spiral arms appear somewhat tightly wound. Evidence of recent or ongoing star formation is apparent within the arms, suggested by the blue-ish coloration. The galaxy's disk appears to be at a slight angle relative to our line of sight. A prominent bar structure is present cutting through the central bulge of the galaxy. The bulge itself is moderately sized relative to the overall disk, but not dominant. There do not appear to be any signs of a major merging event, but there are is evidence of some disturbances in the galaxy structure.
