The galaxy presents as an elongated, edge-on spiral system. A prominent central bulge is visible, exhibiting a concentrated luminosity gradient. The bulge appears somewhat rounded. The disk component is highly inclined to our line of sight, presenting a thin, extended structure. The galaxy displays a smooth, relatively featureless disk, with no immediately apparent signs of active star formation regions or significant dust lanes. The lack of clear spiral arm structure could be a result of the high inclination. Color gradients suggest older stellar populations may dominate the central bulge, while younger populations may be present within the disk. Overall, the galaxy appears to be a relatively quiescent, high-mass spiral galaxy.
