The galaxy presents as a spiral type, exhibiting a distinct disk structure viewed at a slight inclination. Well-defined spiral arms are observable, contributing significantly to the galaxy's overall morphology. These arms appear somewhat flocculent. The galaxy displays a noticeable central bulge, roughly moderate in size compared to the disk. The bulge appears smooth and concentrated, indicative of an older stellar population. The disk shows evidence of ongoing star formation, traced by the presence of bluer regions intermixed with the older stars. Some areas show evidence of disturbances. Overall, the galaxy has an organized structure with a relatively prominent disk and indications of both old and relatively recent star formation activity.
