The galaxy appears as a centrally concentrated, elliptical-shaped object. Its color profile indicates an older stellar population, dominated by yellow-red hues, with negligible blue emission. The light distribution is relatively smooth, lacking any distinct spiral arm structures or prominent dust lanes. There is no obvious evidence of ongoing star formation, instead the light seems to be mostly from old stars. There's a slight asymmetry to the overall shape, but it is very round. The luminosity is very high, which leads to the belief that it is an evolved, massive system. The galaxy seems relatively isolated, with no major signs of tidal interaction or ongoing merger events visible. The edges appear slightly fuzzy.
