The galaxy presents a complex morphology, exhibiting characteristics of both smooth and disturbed systems. The dominant feature is a central, relatively smooth component, possibly a bulge. Superimposed on this are indications of disturbed features. The galaxy appears somewhat rounded in shape, but deviates slightly. There are a few bright knots present, potentially indicative of star-forming regions. These knots seem to be scattered unevenly throughout the galaxy. The galaxy overall displays a bluer hue, suggesting active star formation.
