The galaxy presents a primarily smooth morphology, with a notable lack of distinct spiral arms or a well-defined disk structure. It appears largely elliptical, with an aspect ratio suggesting a nearly spherical shape, although subtle deviations may be present. The galaxy exhibits a central concentration of light, indicative of a galactic nucleus.

Color gradients are discernible, transitioning from a slightly bluer hue in certain regions to a redder central bulge. This suggests variations in stellar populations, with bluer regions potentially indicating areas of more recent star formation, and redder regions suggesting an older stellar population. No signs of major mergers are visible, though a hint of minor disturbance cannot be entirely ruled out. Overall, the galaxy appears to be a relatively undisturbed system.
