The galaxy presents as a somewhat flattened, elliptical system. The light profile appears to be centrally concentrated, exhibiting a smooth, gradual decrease in brightness from the core outwards, suggesting a relatively evolved stellar population. There is a slight elongation, giving it a lens-like shape, though not highly elongated. The galaxy exhibits a reddish hue in the center, with some subtle color variations suggesting areas of relatively recent star formation or differences in metallicity. The overall structure indicates a relatively mature galaxy, with no obvious signs of strong tidal interactions or significant ongoing merger activity, but it is possible that the galaxy experienced a minor merger in the past. Based on the estimated luminosity and color, this galaxy is likely a moderately massive system, with relatively low ongoing star formation.
