The galaxy presents as a disk galaxy, observed nearly edge-on from our vantage point. The disk is elongated, exhibiting a central bulge that appears smooth and somewhat rounded. This central region displays a yellowish-white hue, possibly indicating a population of older stars. The outer regions of the disk show a transition towards bluer colors, hinting at ongoing star formation. No distinct spiral arm structure is discernible. There are no obvious signs of major mergers or significant tidal disturbances. A very thin dust lane may be present bisecting the galaxy.
