The galaxy presents as a singular, relatively smooth, and luminous object. It exhibits a generally elliptical morphology, appearing somewhat elongated rather than perfectly spherical. The central region displays a distinct concentration of light, suggesting a prominent galactic nucleus. The color profile is generally redder, with a slightly yellow hue, indicative of an older stellar population or significant dust content. There is a slight hint of disturbance, possibly indicating a minor interaction or internal activity. Overall, the galaxy's characteristics suggest that it is a relatively massive system with a subdued star formation rate.
