The galaxy presents a relatively smooth, elliptical morphology. Its overall color appears slightly redder than typical spiral galaxies, suggesting a more evolved stellar population. There is no readily apparent disk structure or spiral arm morphology. The light distribution is concentrated towards the center, showing a high degree of central bulge dominance. The galaxy does not exhibit obvious signs of recent or ongoing major mergers. There might be very faint disturbances in its morphology, which indicates that the galaxy may have undergone minor interactions or mergers in the past. The light distribution shows no distinct, separate regions of star formation.
