This galaxy presents as an elongated, disk-shaped structure, likely a spiral galaxy viewed edge-on or a lenticular galaxy. The central bulge appears bright and concentrated, exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. Fainter, bluer light extends along the plane of the disk, suggesting the presence of younger stars and ongoing star formation, although not prominently. The disk appears relatively smooth with some signs of patchiness, but without distinct spiral arms. The galaxy does not exhibit any obvious signs of major mergers or significant tidal disturbances. Overall, it is a moderately luminous galaxy at a redshift of roughly 0.2.
