The galaxy presents as a relatively smooth, concentrated light source with a primarily elliptical morphology. There is some evidence of asymmetry, with the suggestion of a slight extension along one axis, but no obvious spiral structure or bar is apparent. The galaxy exhibits a color gradient, appearing bluer in the central region and trending towards redder hues in the outer parts. No prominent dust lanes or regions of active star formation are visually discernible. Overall, the galaxy appears to be a passively evolving system.
