The galaxy presents as a spiral type, observed at a slight angle relative to edge-on. A central bulge is discernable, appearing relatively small in comparison to the overall disk size.  The spiral arms are not sharply defined, exhibiting a more flocculent or patchy structure.  These arms appear tightly wound around the central bulge. There is some indication of potential asymmetry or a minor disturbance in one of the outer arms. Color gradients suggest a mixed stellar population, with a yellowish central region likely dominated by older stars, transitioning to bluer hues in the outer disk associated with younger, hotter stars. The galaxy does not appear to be undergoing a major merger, however there are possible disturbances present. The galaxy appears to be well resolved for its redshift.
