The galaxy presents a moderately inclined disk orientation. Prominent spiral arms are visible, exhibiting a somewhat flocculent structure. These arms appear relatively open, originating from a central bulge. The bulge itself seems moderate in size, contributing significantly to the overall luminosity. Some disturbance in the morphology is indicated, possibly suggesting ongoing or recent interaction with a smaller galaxy. The galaxy shows colours indicative of ongoing star formation, especially within the spiral arms, as evidenced by the blue hue. A central bar appears absent. Overall, the galaxy exhibits characteristics of a spiral galaxy undergoing active star formation.
