This galaxy presents as a relatively smooth, centrally concentrated object. The core region exhibits a bright, yellowish hue, suggesting an older stellar population is dominant. Moving outward from the center, a fainter, bluer disk-like structure becomes apparent, indicating the presence of younger stars and possibly some ongoing star formation, though the overall star formation rate seems subdued. The galaxy appears somewhat flattened, though not as pronounced as a typical spiral galaxy. There's no strong indication of a major merger event, although there's a slight asymmetry in the extended outer regions, possibly hinting at minor tidal interactions or disturbances. The overall shape tends towards an elliptical morphology but with a discernible disk component.