The galaxy presents as a centrally concentrated object, roughly elliptical in shape, with a smooth, largely featureless appearance. There is a distinct color gradient, transitioning from a yellow-white core to a slightly redder, fainter halo. The core exhibits a high degree of symmetry, with the surrounding halo appearing more diffuse and somewhat irregular in shape. The overall morphology suggests a galaxy dominated by an older stellar population with little evidence of ongoing major star formation or significant dust lanes. There are hints of slight asymmetry in the outer halo, but this could be due to noise or minor tidal interactions. The galaxy does not appear to be undergoing a major merger event.
