The galaxy presents as a largely smooth object with an elliptical morphology. It exhibits a bright, concentrated central bulge. The color profile suggests a relatively evolved stellar population. Fainter, diffuse light extends outward from the core. The overall structure indicates a system with minimal recent or ongoing major mergers. There is no clear spiral arm structure visible. The galaxy appears to be a relatively isolated system with no apparent signs of significant tidal interactions or distortions. The blue color indicates a small amount of star formation may be present.