The galaxy presents a largely smooth morphology, with minimal discernible features such as spiral arms or a prominent disk structure. It appears largely spheroidal, exhibiting a high degree of roundness with only a very slight deviation toward an elongated shape. There is no indication of ongoing major mergers or significant tidal disturbances affecting the system’s structure. The galaxy displays a color gradient, transitioning from a more yellow-orange central region to a slightly bluer hue in the outskirts, indicative of differing stellar populations or dust content across the galaxy. The apparent size is relatively compact, suggesting either a physically small galaxy or one observed at a significant distance, with its estimated size to be around 5 kpc across. The luminosity profile appears relatively smooth and centrally concentrated, characteristic of a more evolved system. The redshift of 0.22 indicates the galaxy is receding from us at a significant fraction of the speed of light, confirming its extragalactic nature and distance.
