The galaxy presents a generally smooth and rounded morphology. There is a notable concentration of light toward the center, suggesting a prominent galactic bulge. The color profile shifts from a yellowish-white core to a fainter, slightly bluer halo. There is no clear evidence of spiral arm structure or significant dust lanes, indicative of a disk galaxy. The overall appearance suggests a relatively evolved system. Given the redshift, the object appears to be a substantial elliptical galaxy with a relatively low star formation rate. There is no obvious signs of a major merging event or tidal disturbance; only a minor possible disturbance.
