The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge with a radial decrease in luminosity. The core displays a yellow-orange hue, suggesting an older stellar population with lower levels of ongoing star formation, possibly dominated by evolved stars. The outer regions are less defined and appear to fade gradually into the background, showing a hint of a more bluish tint, indicating the presence of a younger, though less prominent, stellar population. There is no visually apparent spiral arm structure or significant dust lane obscuration. The overall morphology suggests a system that is not actively undergoing major mergers or disturbances.
