This galaxy appears to be a relatively smooth, elliptical or lenticular type. The light distribution is centrally concentrated, diminishing outwards without any discernible spiral arm structures or a prominent galactic disk. There is a hint of a subtle color gradient, with the core appearing slightly redder compared to the outer regions, possibly indicating a difference in stellar populations. The overall shape is largely spheroidal, with a minimal axis ratio suggesting a somewhat elongated, rather than perfectly circular, form. There is no apparent strong tidal interaction, major disturbance, or ongoing merger activity. Any minor distortions appear to be minimal.
