The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge that appears yellowish in color, suggesting an older stellar population. While appearing mostly smooth, there is a slight hint of asymmetry or subtle features in the outer regions, possibly indicating minor disturbances or interactions. There is a clear lack of defined spiral arms. The color gradients from the core to the outer regions suggest a gradual decline in star formation activity, with the outskirts appearing redder. Overall, the galaxy appears as a passively evolving system with a significant population of older stars and a suppressed rate of star formation.
