The galaxy presents a discernible disk structure, exhibiting a spiral morphology. Two distinct arms emanate from the central region, extending outwards in a somewhat symmetrical fashion. The arms are not tightly wound, suggesting a later-type spiral galaxy classification. Star formation appears to be ongoing, inferred from the subtle blueish hue and slight patchiness within the spiral arms.

The central bulge is moderately sized, contributing significantly to the overall luminosity of the galaxy. Dust lanes are subtly visible within the disk, tracing along the inner edges of the spiral arms. The galaxy displays a relatively smooth appearance, although some irregularities within the arm structure indicate possible minor interactions or disturbances. Overall, the system presents as a well-defined spiral galaxy undergoing active, but not extreme, star formation.
