The galaxy presents a generally smooth morphology, with a subtle elongation suggesting an elliptical shape, or a possible disk galaxy seen at an angle. The central region appears more concentrated and exhibits a yellowish-orange hue, potentially indicating an older stellar population. The outer regions display a bluer tint, which may be due to the presence of younger, hotter stars. There appears to be little evidence of significant spiral arm structure or major disturbances, although a slight asymmetry on one side could indicate a minor interaction or past merger event. Overall, the galaxy seems relatively undisturbed and evolved.
