The galaxy presents as a centrally concentrated, smooth structure. Its light profile suggests a relatively featureless elliptical morphology, lacking prominent spiral arms or a well-defined disk. The light is dominated by redder wavelengths, with a noticeable yellow/gold hue, indicative of an older stellar population and reduced ongoing star formation. The galaxy appears to be fairly isolated, displaying no obvious signs of a major merger event or significant tidal disturbances. There is a slight elongation to its shape, but it appears mostly spheroidal. The galaxy's overall appearance is consistent with a passive, evolved system.
