This galaxy presents as a relatively bright, disk-shaped structure. It displays a prominent central bulge that appears smooth and luminous. The disk component exhibits a complex morphology with evidence of possible spiral arm structures. Some features may suggest minor disturbances. The galaxy's color profile indicates a significant presence of both old and young stellar populations. The overall appearance suggests a system that may be undergoing, or have recently undergone, some form of interaction or internal dynamic process, although further analysis is needed to confirm this.
