The galaxy presents a relatively smooth, elliptical morphology. Its light profile suggests a centrally concentrated structure with a gradual decrease in luminosity outward. The color appears predominantly red/yellow, indicating a population of older stars and a potential lack of significant recent star formation. There is no prominent disk or spiral arm structure visible. Slight irregularitites in color could be evidence of minor interactions or mergers in the past. The apparent round shape suggests that it is seen close to face-on.
