The galaxy appears as a flattened, elongated structure, suggesting a disk-like morphology viewed at a significant inclination. The central region exhibits a concentrated, yellowish-white hue, indicative of an older stellar population, likely a bulge. Fainter, bluer light extends outwards from this core, tracing the spiral arms, although these are not clearly defined due to the viewing angle. These arms indicate areas of ongoing or recent star formation, contributing to the overall light output of the galaxy. The structure is relatively smooth, with hints of disturbance in the outer regions. There is no apparent ongoing major merger. Overall, the galaxy presents characteristics consistent with a spiral or lenticular galaxy at moderate redshift, with both an old stellar population and continued star formation.