The galaxy presents a generally smooth, elliptical morphology, appearing largely spheroidal with minimal discernible disk structure. The light distribution is centrally concentrated, exhibiting a bright, well-defined core that gradually fades outwards. The color profile suggests an older stellar population, with a yellowish-red hue dominating the central region. There is a hint of bluer light in the surrounding halo, possibly indicating some recent star formation at the periphery, but it's subdued. The galaxy shows no obvious signs of major mergers or tidal disturbances, although some subtle asymmetries in the outer isophotes could potentially indicate minor gravitational interactions. Overall, the galaxy appears to be a relatively massive, evolved system with a quiescent star formation history.
