The galaxy presents as a spiral galaxy, displaying a prominent disk structure. Two distinct spiral arms emanate from a central, moderately sized bulge. These arms exhibit a medium winding, not tightly wound nor exceptionally loose. The presence of a bar feature appears strong within the central region of the galaxy, bisecting the bulge and influencing the arm structure.

Color variations within the disk suggest ongoing star formation, with bluer regions indicating areas of active stellar birth. The overall morphology hints at a relatively massive galaxy, with intermediate star-forming activity. There may be minor disturbances hinting at a past or ongoing minor merger event.
