The galaxy presents as a centrally concentrated, smooth system. It exhibits a roughly elliptical morphology, appearing mostly round with a slight deviation from perfect circularity. There is a clear concentration of light towards the center, indicative of a bulge component. The color profile suggests a dominant older stellar population, with the central regions appearing more yellow/red than the outer areas. Evidence of spiral arm structure or significant star formation regions are not apparent. Overall, the galaxy appears relatively undisturbed, showing no signs of major merger events or significant tidal interactions. The overall structure is relatively compact.
