The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing largely featureless with a high degree of radial symmetry. The light profile suggests a dominant spheroid component. There is a slight elongation, deviating marginally from a perfectly circular shape.

The galaxy displays a subtle color gradient, with the central region exhibiting a somewhat yellower hue, possibly indicating an older stellar population. Moving outwards, the outer regions appear slightly bluer, perhaps indicating the presence of younger stars. This subtle color variation suggests a degree of stellar population diversity within the galaxy.

Overall, the galaxy appears as a relatively quiescent system, displaying minimal signs of ongoing star formation or recent interaction.
