The galaxy presents as an elliptical morphology, elongated in shape, with a smooth, diffuse light distribution. A color gradient is present, with a central region exhibiting a yellow-orange hue indicative of an older stellar population or significant dust extinction. The outer regions appear bluer, suggesting the presence of younger stars, or less dust. There is no obvious indication of spiral arms or a distinct disk structure; the overall form is relatively featureless. The light tapers off gradually from the central region to the edges, consistent with a well-mixed stellar population and/or a smooth dust distribution. There are no strong signs of tidal disturbances or interactions. The overall appearance suggests a galaxy that has undergone significant evolution, likely with ongoing, but relatively low, star formation.
