The observed galaxy presents as a spiral galaxy with a prominent bar structure. The spiral arms appear well-defined, exhibiting a flocculent morphology with noticeable star formation regions along the arms, characterized by a bluish hue indicative of younger stellar populations. The bulge component is relatively small, appearing subdued compared to the disk. The disk dominates the overall visual impression of the galaxy, with a relatively high degree of symmetry and order. There is no apparent major interaction or significant tidal disturbance visible.
