The galaxy presents as a somewhat elliptical, relatively compact object. It exhibits a smooth light distribution, with a central concentration of luminosity that gradually decreases towards the outer edges. The color profile suggests an older stellar population, as it appears with a yellow-orange hue. There is no visible evidence of spiral arm structure or significant dust lanes. Overall, the morphology is consistent with an elliptical galaxy at a redshift of approximately 0.32, indicating that we are observing it at a considerable distance. Its size is typical for galaxies at its redshift, and its calculated mass is relatively high. The rate of star formation is relatively low, which also agrees with the color of the galaxy.
