The galaxy appears as a centrally concentrated object with a smooth, elliptical morphology. There's a slight elongation, though it is close to round, with no discernible spiral arm structure or prominent disk. The light profile suggests a fairly homogeneous stellar population, potentially dominated by older stars. The galaxy exhibits a color gradient, appearing somewhat bluer in the central regions, potentially indicating some degree of recent or ongoing star formation in that area, though it is still overall a relatively redder galaxy. The presence of a relatively smooth structure, the slight color gradient, and lack of any major disturbances or indications of significant recent mergers suggests it is a relatively relaxed galaxy, potentially a lenticular or an elliptical galaxy that has reached a relatively stable state after experiencing some past merger.
