The galaxy presents as a highly elongated, spindle-shaped structure. A dominant central bulge appears yellowish-white, suggesting an older stellar population. Surrounding the bulge, a flattened disk is visible, displaying a bluer hue. This indicates the presence of younger, hotter stars.

The disk exhibits a generally smooth appearance, lacking prominent spiral arm structures or distinct star-forming regions. The galaxy appears relatively undisturbed, without evidence of ongoing major mergers or significant tidal interactions. There might be some very minor disturbances.

The estimated physical size, implied by the apparent angular size and redshift, suggests that it is a substantial galaxy. Its spectral properties further suggests a large mass and moderate rate of star formation for its age.
