The galaxy presents as a lenticular or possibly a spiral galaxy seen nearly edge-on. A prominent central bulge is visible, exhibiting a yellowish-orange hue, which suggests a population of older stars. The galaxy displays a distinct disk component. The disk itself appears relatively smooth with no obvious spiral arm structures discernible at this resolution. There is a subtle color gradient within the disk, with slightly bluer regions observed towards the outer edges, potentially indicating the presence of younger stars. Dust obscuration appears minimal. No significant signs of tidal disturbances or ongoing mergers are readily apparent.
