The galaxy presents an elliptical morphology, appearing elongated with a smooth, featureless light distribution. The central region exhibits a bright, concentrated luminosity, possibly indicative of a substantial stellar population or an active galactic nucleus. The galaxy displays a gradual decrease in luminosity from the core outwards, suggesting a radial density gradient in its stellar distribution. There is a subtle color gradient noticeable, with the central region appearing more yellow/white, and the outer regions exhibiting a bluer hue. This could be the result of an aging stellar population in the core, and the star formation region located away from the center. There appears to be a slight warping in the structure, which is visible in the lower left corner. This warp is a possible indication of a gravitational interaction with another galaxy or past galactic merger.
