The galaxy presents an overall elliptical morphology, with a smooth, largely featureless appearance. The central region exhibits a bright, concentrated luminosity profile, suggesting a prominent galactic nucleus. The light distribution flattens towards the outer regions of the galaxy, but there is no dust apparent in the image. The color gradients show a progression from yellowish in the central bulge to somewhat bluer hues toward the outer regions, indicating a possible transition from older stellar populations to younger, hotter stars in the outskirts, despite the galaxy's smooth morphology. There appears to be a slight asymmetry, perhaps indicating a possible minor gravitational interaction in its past. The shape is elongated, departing significantly from a spherical structure.
