The galaxy exhibits a concentrated, centrally bright morphology. It appears mostly smooth, with an elliptical shape. The central region shows a yellowish-white hue, which likely indicates an older stellar population. There is a slight gradient in color moving outward from the center, with a subtle transition to a redder tone in the outer regions, possibly due to dust or a change in the composition of stars. No distinct spiral arms or bar structures are readily visible. The overall impression is that of a relatively quiescent system.
