The galaxy presents a concentrated, elliptical morphology. It exhibits a smooth, featureless appearance, lacking prominent spiral arms or a distinct disk structure. The central bulge appears dominant and is a yellow-white hue, suggesting a population of older stars. The outer regions of the galaxy display a subtle color gradient towards redder hues, implying the presence of a more aged stellar population or dust obscuration in these areas. The galaxy does not appear to be undergoing any major interactions or mergers, with no obvious tidal tails or significant distortions in its shape.
