The galaxy presents as a relatively smooth, elliptical-like object. Its light profile appears centrally concentrated, with a gradual decrease in intensity outwards from the core. There is a slightly oblate spheroidal shape, verging on perfectly circular. The galaxy exhibits a broad spectral energy distribution, with flux detected across green, red, and infrared wavelengths, suggesting a diverse stellar population. There is no clear evidence of spiral arms or other disk features. The galaxy exhibits no obvious signs of ongoing major mergers or strong tidal disturbances, although subtle asymmetries cannot be ruled out at this resolution. Overall, the galaxy appears to be a relatively undisturbed, evolved system.
