The galaxy presents as a slightly elliptical structure, appearing relatively smooth in texture. There is a distinct central bulge that is more luminous than the surrounding galactic disc. The light distribution diminishes gradually from the center outwards, showing no obvious spiral arm structures or prominent dust lanes. The galaxy appears nearly edge-on. Its light is primarily concentrated in the central region, with a more diffuse halo extending outwards. The overall color profile is indicative of a mature stellar population. The morphological characteristics are consistent with an early-type spiral or a lenticular galaxy. Evidence suggests an ongoing but relatively low star formation rate. Based on morphological classifications, there appears to be no major merging activity, but there may be evidence of minor disturbances.
