The galaxy presents a generally smooth morphology, with a slight elongation suggesting an intermediate shape between elliptical and lenticular. Its color profile indicates a dominant population of older stars, likely with limited ongoing star formation. There is subtle color variation, with a hint of blue-green tinges concentrated in certain areas suggesting possible localized regions of younger stellar populations or emission nebulae. The overall structure is fairly undisturbed, showing no obvious signs of major mergers or tidal interactions. A degree of asymmetry may be present, but this is not well-defined and could be attributed to noise or minor internal structures.
