The galaxy presents as an edge-on disk galaxy with a prominent central bulge. The bulge appears luminous and smoothly distributed, transitioning into a relatively thin disk. The disk component exhibits signs of structure and patchiness, which may indicate ongoing star formation, but that is difficult to ascertain from this imagery. There is very little indication of merging features or tidal tails, suggesting the galaxy is relatively undisturbed. The disk appears to be slightly warped, or perhaps is at an angle, so that one side of the galaxy appears closer to the camera than the other. The colour of the galaxy is generally redder in the bulge and centre, suggesting a greater population of older stars, transitioning to slightly bluer hues in the outer disk regions. There is little to no evidence of a strong dust lane along the galactic plane.
