The galaxy presents as an elongated, disk-shaped structure, observed nearly edge-on. There's a noticeable central bulge that appears somewhat boxy, contributing to the galaxy's overall luminosity. The disk itself exhibits a smooth texture with little apparent structure such as spiral arms or distinct dust lanes. The galaxy appears to be transitioning to a more passive state of star formation, indicating an aging stellar population. There's no clear evidence of major mergers or significant tidal disturbances in the image, but possible minor distortions of the disk may suggest previous minor interactions with other galaxies.
