The galaxy presents a generally smooth morphology with a slight elliptical shape. It appears to be a disk-dominated system. The light distribution is centrally concentrated, fading gradually toward the edges. A subtle color gradient is observed, with a central region exhibiting a yellower hue, suggesting an older stellar population. The outer regions are slightly bluer, possibly indicating some ongoing, albeit limited, star formation. No strong spiral arm structures or prominent dust lanes are visible, which supports the assessment of a relatively smooth, evolved galaxy. There are no indications of any major merging events, though some minor disturbances cannot be fully ruled out at this resolution. The galaxy is positioned at a cosmological redshift, indicating a significant distance.
