This galaxy presents as a spiral system, viewed at a high inclination. The disk component appears quite prominent, exhibiting clear spiral arm structure. The arms are not tightly wound, showing a more open configuration. Star formation activity is likely occurring within these arms.

A central bulge is discernible, although it appears relatively small in proportion to the overall disk size. There is no indication of a strong bar-like structure within the central region; instead, the nuclear region is relatively smooth. The morphology is somewhat disturbed, there might be a minor interaction.
