The galaxy presents as a centrally concentrated system with a smooth, elliptical morphology. There is minimal evidence of distinct spiral arms or a pronounced disk structure. The light distribution suggests a relatively even stellar population throughout the galaxy, with a somewhat concentrated, bright central region. The overall color appears to be red-shifted, indicating an older stellar population, with the yellow/orange hue arising from evolved stars. There are no obvious signs of ongoing major mergers or significant tidal disturbances. The morphology aligns with an early-type galaxy classification, exhibiting properties consistent with an elliptical galaxy at a moderate distance.
