The galaxy presents as a moderately luminous, elongated structure. The morphology is suggestive of a disk galaxy viewed at a significant inclination. The central region exhibits a yellowish hue, potentially indicative of an older stellar population or dust obscuration. Towards the outer regions, a bluer color is apparent, suggestive of more recent star formation. The disk is relatively smooth, lacking prominent spiral arm structures in this image. There is slight asymmetry in the overall shape, hinting at possible gravitational interactions or past merger events, though no major disturbances are immediately obvious. The size appears moderate, consistent with a typical spiral or lenticular galaxy. The object is significantly redshifted, indicating a substantial distance.
