The galaxy presents as an edge-on disk galaxy with a notable central bulge. The bulge exhibits a yellow-orange hue, suggesting a population of older stars with lower levels of on-going star formation within the bulge region.

The disk component appears relatively thin and elongated, displaying a bluer color profile than the bulge. Faint dust lanes are suspected, creating slightly mottled appearances across the face of the disc. The overall morphology suggests a relatively undisturbed system, lacking significant tidal features.

In summary, the galaxy is most likely a quiescent spiral galaxy with a prominent bulge and well-defined disk structure, seen nearly edge-on.
