The observed galaxy exhibits a pronounced central bulge, characterized by a high concentration of older stellar populations, indicated by its yellowish hue. Faint spiral arms extend from the central bulge, but they are not well-defined. The disk is viewed at a slight angle, but it is mostly face-on. Overall, the light is smooth suggesting older stellar populations. The galaxy is relatively massive, with a low star formation rate. There is no evidence of any significant ongoing mergers or major disturbances. The galaxy possesses a moderate-sized bulge. A prominent central bar appears to be present. The galaxy is estimated to be approximately 8.7 kpc in radius.
