The galaxy presents an elliptical morphology, appearing as a smooth, centrally concentrated object. The central region exhibits a yellowish-orange hue, suggesting a population of older stars. The outer regions transition towards a fainter, greenish tint, possibly indicating the presence of younger stellar populations or ongoing, albeit limited, star formation. There is no prominent disk structure or spiral arm features discernible. The overall shape indicates it is unlikely to be a spiral galaxy. The galaxy displays a relatively undisturbed structure, showing no evidence of major mergers or significant tidal distortions. Minor disturbances cannot be ruled out, but no clear signs of ongoing interaction are immediately visible. The object's apparent roundness suggests a classification closer to an elliptical galaxy as opposed to a lenticular galaxy.