The observed galaxy presents an edge-on disk morphology. It exhibits a prominent central bulge that appears somewhat rounded. The disk is relatively smooth in appearance, showing minimal signs of significant star formation regions or spiral arm structures that are often associated with grand design spirals. The galaxy does not appear to be undergoing any major merger events, although subtle disturbances or tidal features may be present at a low level. The colour suggests a population of older stars, particularly in the bulge.
