The galaxy appears to be a spiral type, presenting a disk-like structure viewed at a slight angle. It exhibits two prominent spiral arms that emanate from a central region, which may host a bar-like feature. The arms display a somewhat flocculent structure with varying degrees of tightness in their winding. The bluer hue of the arms suggests active star formation regions. The central bulge seems relatively small compared to the overall size of the disk. There is a possibility of some minor disturbance in the galaxy's morphology, perhaps due to a minor gravitational interaction. However, a dominant merging event is not apparent. Overall, the galaxy exhibits characteristics of a normal spiral galaxy with ongoing star formation.
