The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits a nearly circular morphology. A slightly brighter yellowish hue is observed toward the galactic center, suggesting a concentration of older stellar populations in the bulge. Fainter, diffuse light extends outwards from the core, decreasing in intensity with radial distance. No distinct spiral arm structures or significant dust lanes are visible. Overall, the galaxy exhibits characteristics consistent with an elliptical morphology. The galaxy is moderately luminous with a redshift of z = 0.219265, indicating a substantial distance. There may be some minor disturbance occurring.
