The galaxy presents a generally smooth, elliptical morphology. There's a centrally concentrated bright nucleus, suggestive of an older stellar population. The outer regions exhibit a more diffuse appearance, with a slight elongation suggesting it is not perfectly spherical. Faint blue hues can be seen near the center of the galaxy, suggesting it may still be forming stars at a low rate. There is no obvious spiral structure or dust lanes visible. It shows no obvious signs of ongoing major mergers or tidal disturbances. The galaxy appears relatively isolated, lacking close companion galaxies that might influence its morphology.
