The galaxy appears to be a faint, relatively small spiral galaxy, seen at an oblique angle. A slight bulge is visible in the center with what seems to be loosely wound arms extending outwards, indicating the presence of a disk structure. The galaxy's color is predominantly blue, suggesting a population of young, hot stars within its spiral arms. Some faint redder regions are also visible, potentially indicating the presence of older stellar populations or dust lanes. There are some possible signs of minor disturbances in the structure. The galaxy is not undergoing a major merger, but may be undergoing a minor merger. Overall, the galaxy exhibits a non-smooth morphology and may be disturbed, with a weak, possible disk and faint features.
