The galaxy appears to be a relatively smooth, elliptical structure with a concentrated central bulge. The color gradient suggests a population of older stars dominating the core, exhibiting a yellowish-orange hue. A fainter, bluer component is visible in the outer regions, possibly indicating more recent or ongoing star formation, though the image resolution limits detailed assessment. The overall morphology implies that this system is likely an early-type galaxy. No significant tidal features or signs of a major merger event are readily apparent.
