This galaxy appears to be a relatively compact object. The light profile suggests a smooth and centrally concentrated morphology, with a dominant bulge component. There is faint evidence of a very small disc surrounding the main bulge, but the bulge appears to comprise most of the galaxy. The galaxy appears yellow, suggestive of an older stellar population. The low star formation rate suggests that the galaxy is relatively quiescent, with minimal ongoing star formation activity. There are no major tidal features present, suggesting the galaxy is not undergoing any major mergers. Overall, this galaxy presents as a fairly undisturbed system, dominated by an evolved stellar population within a smooth bulge.
