The galaxy presents a mostly smooth, elliptical appearance with a concentrated central bulge. A smaller, adjacent component is present, indicating a potential interaction or merger event. The primary galaxy exhibits a yellowish-white hue, suggesting an older stellar population and diminished star formation. Slight irregularities in the outskirts hint at past or ongoing gravitational disturbances. Overall, the morphology leans toward a relaxed, spheroid-dominated system, but with a degree of structural complexity possibly arising from external influences.
