The galaxy presents as a spiral structure with a relatively bright central bulge. The spiral arms are loosely wound and appear to be composed of numerous star-forming regions, giving them a somewhat clumpy appearance. There are hints of two primary arms with some fainter, less defined arm structures. The galaxy exhibits a slightly elongated shape. The overall color is bluish, which suggests a younger stellar population and ongoing star formation, though it does have a general yellowish glow from its core, showing the existence of an older population of stars. There appears to be a small degree of apparent asymmetry, with one side having a more extended or disrupted appearance, potentially indicative of a minor interaction or merger event. A central bar may be present though this feature is hard to define.
