The galaxy presents as a relatively compact object with a smooth, elliptical morphology. It exhibits a concentrated central bulge that is brighter than the surrounding regions. The color gradient suggests an older stellar population, primarily concentrated toward the center, with a yellow-red hue. There is no clear evidence of spiral arms, a disk component, or significant dust lanes. The galaxy appears undisturbed, without any signs of tidal tails or ongoing major mergers, although a minor disturbance cannot be completely ruled out. Based on the colors, the galaxy is likely in a quiescent or passively evolving state with a relatively low star formation rate. The overall appearance is consistent with an elliptical galaxy at a moderate redshift.
