The galaxy presents as an edge-on spiral system with an elongated, disk-like structure. A prominent central bulge is evident, exhibiting a brighter, more concentrated luminosity. The bulge appears relatively smooth and rounded in morphology. The disk component shows hints of dust lanes running along the equatorial plane, although these features are somewhat obscured by the edge-on viewing angle. There is a subtle bluing towards the outer edges of the disk, potentially indicative of younger stellar populations and ongoing star formation activity. The galaxy does not appear to be undergoing any major merger events or significant tidal disturbances, suggesting a relatively quiescent state.
