The galaxy presents as a spiral type. It exhibits a disk-like structure with moderate arm definition, though these arms are fragmented and not continuously wound. The winding appears to be medium and the arms seem to have about 2 arms that extend from the center. A weak bar structure may be present at the galaxy's core, though it is difficult to discern definitively due to the inclination and resolution. The bulge is moderately sized relative to the disk. There may be some minor disturbances in the galaxy's morphology, potentially indicating a past or ongoing interaction. The galaxy shows a color gradient, with a bluer hue in the spiral arms suggesting active star formation and a redder central bulge potentially indicating an older stellar population.
