The galaxy presents as a largely featureless elliptical, displaying a smooth and rounded morphology. The color profile indicates a yellowish hue that is indicative of an older stellar population. No prominent spiral arms or dust lanes are apparent. The galaxy lacks sharp defined edges and gradually fades into the background sky, which is consistent with light from older stars. There is no evidence of active galactic nuclei activity or recent major merger events from the overall structure. Minor disturbances may be present but aren't clearly visible. It appears quite compact in size.
