The galaxy presents a smooth, elliptical morphology. It exhibits a bright, concentrated core that fades outwards. The color profile suggests a relatively old stellar population, likely dominated by redder stars, with a hint of bluer light in the central regions. No distinct spiral arms or other features associated with ongoing disk star formation are apparent. The galaxy appears relatively isolated, without evidence of significant tidal interactions or mergers. The shape is close to round, with some elongation visible.