The galaxy presents as a spiral type, observed at a moderate redshift. The disk component exhibits a relatively high degree of organization with apparent spiral arm structures. These arms appear tightly wound close to a prominent bulge.

The bulge is noticeably bright and yellow, possibly indicating an older stellar population. The spiral arms show a bluer hue, consistent with ongoing star formation. There is a suggestion of an inner bar structure in the central region.

There is a possibility of a minor gravitational interaction occurring with a nearby galaxy, given the slight asymmetry of the disk and subtle disturbances. The apparent size suggests a galaxy of considerable physical dimension.
