The observed galaxy presents as a spiral type. A prominent bar structure is visible, transecting the central bulge. The bulge appears relatively small, gradually fading into the spiral arms. The spiral arms are well-defined, with a dominant two-arm structure exhibiting medium winding. Star formation appears to be present within the spiral arms, indicated by subtle variations in color. There are no obvious signs of major mergers, though subtle asymmetries could indicate minor interactions or disturbances. The galaxy is not observed edge-on, with the disk clearly presented.
