The galaxy appears to be a relatively smooth, disk-like structure with an elliptical shape. It exhibits a central bulge that is more luminous and concentrated, suggesting a higher density of older stars. The color gradient transitions from a yellowish-orange core to bluer hues in the outer disk. The outer regions of the galaxy appear somewhat fainter and diffuse. There is a suggestion of spiral arm structure, but it is not well-defined. There may be some minor disturbances in the structure which could indicate a past or ongoing minor merger event. 
