This galaxy presents as a spiral type, with tightly wound arms emanating from a bright, somewhat diffuse central bulge. The spiral arms exhibit a clumpy morphology, suggesting regions of active star formation. The color is predominantly blue, indicating a relatively young stellar population and ongoing star formation. The galaxy shows no signs of a strong bar structure. There may be a second galaxy either colliding or being gravitationally distorted into the spiral galaxy. There may be an interaction or merger event occurring that is creating an irregular shape for the galaxy. The galaxy appears to be in a relatively isolated environment, showing little evidence of tidal interactions with other nearby galaxies, except possibly the small galaxy on the left. The overall appearance is consistent with a galaxy undergoing active star formation within its spiral arms.