The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a concentrated, bright core with a distinct reddish-orange hue. Moving outwards from the core, the galaxy displays a gradual decrease in surface brightness. The outer regions appear to have a slightly bluer tint than the core. There is no definitive evidence of spiral arms or a well-defined disk structure from this particular image. Small signs of disturbances and merging are also not present. The light distribution suggests a relatively evolved stellar population in the core, possibly indicative of older stars, while the outer regions might contain a younger stellar population.
