The galaxy presents a largely smooth, elliptical morphology. Its color profile exhibits a central concentration of reddish hues, suggesting an older stellar population dominates the core, with less active star formation. The outer regions transition toward a more yellowish color, possibly indicating the presence of a younger stellar population, albeit less pronounced. The overall symmetry of the galaxy is slightly disturbed by a faint extension, hinting at possible minor gravitational interactions or disturbances. It does not appear to be undergoing a major merger. The galaxy has a fairly compact apparent size, suggesting it is relatively distant.
