The galaxy presents as a spiral type, with a prominent, though not centrally dominant, bulge. Two tightly wound spiral arms are clearly visible, exhibiting a continuous pattern. The disk component appears significant, contributing heavily to the overall light. The galaxy does not appear to be viewed perfectly face-on, presenting at a slight inclination. The central bulge exhibits a yellow-red hue, suggesting an older stellar population. The spiral arms show a bluer tint, indicative of ongoing star formation. There is evidence of a potential interaction or merger event, visible as some disturbance in the main structure of the galaxy. The galaxy exhibits a weak bar feature crossing the central region.
