The observed galaxy presents as a spiral type, characterized by prominent spiral arms emanating from a central bulge. The spiral arms are well-defined, exhibiting a dual-armed structure. A bar-like feature appears to traverse the galactic center, exhibiting some definition. The winding of the arms appears intermediate, neither tightly wound nor exceptionally loose.

The galaxy's color profile suggests a mix of stellar populations. The central bulge exhibits a yellower hue, indicating the presence of older stars. The spiral arms are bluer, indicative of ongoing star formation.

The morphological integrity of the galaxy appears largely undisturbed, showing no visual indicators of a major merger event, although some minor irregularities might be present, potentially hinting at past gravitational interactions. The galaxy is viewed at an angle, but its overall disk structure is still apparent.
