The galaxy presents a largely elliptical morphology. The light distribution appears relatively smooth and concentrated towards the center, indicating a substantial bulge component. Some subtle variations in color are observable across the galaxy, suggesting variations in stellar populations or dust content. There are no clear signs of strong spiral arm structure or major disturbances, although very faint features hint at possible minor interactions or internal structures. The overall appearance is consistent with a galaxy undergoing relatively low levels of star formation. The galaxy's color suggests a redder spectral energy distribution in comparison to actively star-forming galaxies.
