The galaxy appears as a largely featureless, elliptical object, with a smooth, concentrated light profile. The core exhibits a yellowish-orange hue, which gradually fades into a greenish tint at the outer edges. There is no evidence of spiral arms or a distinct disk structure. The galaxy's form is generally round, showing no signs of significant tidal disruption or major ongoing mergers. Minor disturbances might be present, but the overall morphology suggests it is likely a relaxed system with no major interactions at the moment. The color distribution suggests a population of older stars, and possibly some ongoing star formation activity.
