The galaxy presents a largely smooth morphology. There is a slight deviation from perfect circularity, appearing somewhat elliptical in shape. The light distribution is centrally concentrated with a gradual decrease in brightness outwards. The core of the galaxy has a yellow-orange hue, suggesting a significant population of older stars. The outer regions appear marginally bluer than the core, suggestive of a small amount of more recent star formation relative to the core. There are no obvious spiral arm structures or bar features. Based on its appearance, the galaxy is likely a massive elliptical galaxy with a relatively high degree of spheroidal symmetry and low specific star formation rate. There is no indication of ongoing major mergers or significant tidal disturbances.
