The galaxy presents a primarily blue hue, indicating relatively recent or ongoing star formation. It exhibits a somewhat irregular morphology, appearing as a disturbed disk galaxy seen at a slight angle. Spiral arms are visible, though not well-defined, suggesting they are either faint, tightly wound, or disrupted. A central bulge can be discerned, though it does not appear to dominate the overall structure. The light distribution across the galaxy is moderately concentrated, with the central region being brighter than the outer regions. Overall, the galaxy displays characteristics indicative of potential interactions or minor merging events, contributing to its irregular shape and ongoing star formation activity.
