This galaxy appears to be a relatively smooth, elliptical galaxy. The object exhibits a concentrated central bulge with a gradual decrease in luminosity outward. There is minimal evidence of spiral arm structures or significant dust lanes, suggesting a lack of active star formation. The object's smooth morphology and lack of major disturbances indicates it is likely not undergoing a major merger event. There is a slight elongation along one axis, suggesting a shape that deviates from a perfect sphere, but the dominant characteristic is that of a spheroidal system. The color appears relatively uniform across the galaxy, with a slightly redder hue overall, indicative of an older stellar population.
