The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing more elongated than perfectly circular, with a hint of disk-like structure. The light profile suggests a lack of prominent spiral arms or distinct features, indicating a predominantly older stellar population. The central region appears brighter and more densely packed with stars. There's little evidence of active star formation based on the color, which is more consistent with evolved stars and a low star formation rate. There is no current major merger activity observed.
