The galaxy appears as an elliptical, somewhat elongated structure. Its color profile suggests a concentration of older stars in the central bulge, indicated by a yellow-orange hue which fades smoothly toward the periphery. A notable absence of distinct spiral arms or prominent dust lanes suggests that this galaxy is likely an early-type galaxy. There are no strong indications of active star formation within the galaxy. The overall morphology suggests a relatively smooth, evolved system with minimal signs of recent mergers or major disturbances.
