The galaxy appears as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing somewhat rounded in shape with a slight elongation. The core region displays a bright, condensed central bulge. The color profile suggests a dominant older stellar population, as the galaxy exhibits a yellow-red hue throughout. There is a hint of blueish light emanating from the outer regions. It is difficult to discern any distinct spiral arm structure. The overall structure suggests minimal ongoing star formation. There are no major indications of significant tidal disturbances or ongoing mergers. Overall, the galaxy appears to be an evolved system with a high degree of central concentration and a predominantly smooth, featureless structure.
