The galaxy presents a relatively smooth, elliptical morphology. Its light is concentrated toward the center, with a gradual decrease in surface brightness moving outward, resulting in a fairly round appearance. There is no readily apparent disk structure or spiral arm features. The color gradient suggests a population of older stars, with a redder hue in the central regions, indicating a potential lack of ongoing significant star formation. There are no signs of major mergers or tidal disturbances present. The overall light distribution is indicative of a fairly relaxed, undisturbed system.
