The galaxy presents as a spiral, viewed at an oblique angle, with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting a population of older stars. Faint spiral arms are visible, though their structure is not sharply defined. The arms appear somewhat tightly wound. Patches of blueish color can be discerned within the disk, potentially indicating regions of active star formation. The overall morphology hints at a well-formed spiral structure, despite the image resolution limitations. There is no obvious indication of any major mergers or strong tidal disturbances within the image frame.
